0000000000074812

AUTHOR

Rebecca Azulay

0000-0002-2200-5393

showing 24 related works from this author

First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring

2019

The Event Horizon Telescope (EHT) has mapped the central compact radio source of the elliptical galaxy M87 at 1.3 mm with unprecedented angular resolution. Here we consider the physical implications of the asymmetric ring seen in the 2017 EHT data. To this end, we construct a large library of models based on general relativistic magnetohydrodynamic (GRMHD) simulations and synthetic images produced by general relativistic ray tracing. We compare the observed visibilities with this library and confirm that the asymmetric ring is consistent with earlier predictions of strong gravitational lensing of synchrotron emission from a hot plasma orbiting near the black hole event horizon. The ring rad…

Magnetohydrodynamics (MHD)010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizongalaxies: jetAstronomyStrong gravitational lensingblack hole physicsjets [galaxies]galaxies: individualAstrophysicsaccretion accretion disk01 natural sciencesGeneral Relativity and Quantum CosmologyGalaxies: individual (M87)accretion010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsaccretion accretion disksaccretion diskshigh angular resolution [techniques]Accretion disks(MHD)Astrophysics - High Energy Astrophysical PhenomenaGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Compact stargalaxies: individual: M87magnetohydrodynamics (MHD)Techniques: high angular resolutionGeneral Relativity and Quantum Cosmology0103 physical sciences(M87)0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeAstronomy and AstrophysicsBlack hole physicsAstrophysics - Astrophysics of Galaxiesblack hole physicBlack holeRotating black holeSpace and Planetary Sciencemagnetohydrodynamics: MHDGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)magnetohydrodynamics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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THEMIS: A Parameter Estimation Framework for the Event Horizon Telescope

2020

This is an open access article.-- Full list of authors: Broderick, Avery E.; Gold, Roman; Karami, Mansour; Preciado-López, Jorge A.; Tiede, Paul; Pu, Hung-Yi; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Baloković, Mislav; Barrett, John; Bintley, Dan; Blackburn, Lindy; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Cho, Ilje; Conway, John E.; Cordes, James M.; Crew, Geoffrey B.; Cu…

010504 meteorology & atmospheric sciencesExploitAstronomy01 natural sciencesData typeSet (abstract data type)Galactic center0103 physical sciencesVery-long-baseline interferometry16471769010303 astronomy & astrophysics0105 earth and related environmental sciencesVery long baseline interferometryPhysicsEvent Horizon TelescopeSupermassive black holeAstrophysical black holesGalactic CenterAstronomy and Astrophysics98565Black hole[SDU]Sciences of the Universe [physics]Space and Planetary ScienceAstronomy data analysis1858[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]AlgorithmSubmillimeter astronomy
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Gravitational Test beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole

2020

All authors: Psaltis, Dimitrios; Medeiros, Lia; Christian, Pierre; Özel, Feryal; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca; Ball, David; Baloković, Mislav; Barrett, John; Bintley, Dan; Blackburn, Lindy; Boland, Wilfred; Bower, Geoffrey C.; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chan, Chi-kwan; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Cho, Ilje; Conway, John E.; Cordes, James M.; Crew, Geoffrey B.; Cui, Yuzhu; Davelaar, Jordy; De Laurentis, Mariafelicia; Deane, Roger; Dempsey, Jessica; Desvign…

High Energy Astrophysical Phenomena (astro-ph.HE)Event Horizon TelescopePhysicsGravitational waveAstronomyKerr metricFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Gravitation and Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyBlack holeGravitationGeneral Relativity and Quantum Cosmology0103 physical sciencesMetric (mathematics)Shadow[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Statistical physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaParametric statisticsPhysical Review Letters
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First M87 Event Horizon Telescope Results. II. Array and Instrumentation

2019

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ~1.3 mm, EHT angular resolution (λ/D) is ~25 μas, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of th…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonAstronomyAstrophysics::High Energy Astrophysical Phenomenainterferometers [instrumentation]black hole physicsFOS: Physical sciencesgalaxies: individualGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciencesGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)instrumentation: interferometer0103 physical sciencesVery-long-baseline interferometryAngular resolutionInstrumentation (computer programming)instrumentation: interferometers010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy Astrophysics0105 earth and related environmental scienceshigh angular resolution [echniques]Event Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Supermassive black holeGalaxy: centerhigh angular resolution [techniques]Astronomytechniques: high angular resolutiongravitational lensing: strongAstronomy and Astrophysicscenter [Galaxy]Hydrogen maserblack hole physicAstrophysics - Astrophysics of Galaxiesechniques: high angular resolutionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)strong [gravitational lensing]MillimeterAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]The Astrophysical Journal Letters
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Radio detection of the young binary HD 160934

2013

Precise determination of dynamical masses of pre-main-sequence (PMS) stars is essential to calibrate stellar evolution models that are widely used to derive theoretical masses of young low-mass objects. Binary stars in young, nearby loose associations are particularly good candidates for this calibration since all members share a common age. Interestingly, some of these young binaries present a persistent and compact radio emission, which makes them excellent targets for astrometric VLBI studies. We aim to monitor the orbital motion of the binary system HD 160934, a member of the AB Doradus moving group. We observed HD 160934 with the Very Large Array and the European VLBI Network at 8.4 an…

Orbital elementsPhysicsEuropean VLBI NetworkAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceVery-long-baseline interferometryOrbital motionBinary starAstrophysics::Solar and Stellar AstrophysicsStellar evolutionAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)AB Doradus moving group
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Radio emission in ultracool dwarfs: the nearby substellar triple system VHS 1256$-$1257

2018

Aims. With the purpose of investigating the radio emission of new ultracool objects, we carried out a targeted search in the recently discovered system VHS J125601.92-125723.9 (hereafter VHS 1256-1257); this system is composed by an equal-mass M7.5 binary and a L7 low-mass substellar object located at only 15.8 pc. Methods. We observed in phase-reference mode the system VHS 1256-1257 with the Karl G. Jansky Very Large Array at X band and L band and with the European VLBI Network at L band in several epochs during 2015 and 2016. Results. We discovered radio emission at X band spatially coincident with the equal-mass M7.5 binary with a flux density of 60 μJy. We determined a spectral index α …

Magnetic field - radiation mechanismsPhysicsInterferometric010504 meteorology & atmospheric sciencesTriple systemBrown dwarfFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral - techniques01 natural sciencesBrown dwarfs - starsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciences
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First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

2019

We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ~40 μas, consistent with the size and shape of the lensed photon orbit encircling the "shadow" of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others' work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to av…

Brightness010504 meteorology & atmospheric sciencesgalaxies: jetAstronomyblack hole physicsFOS: Physical sciencesgalaxies: individualtechniques: image processingAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciencesSynthetic dataGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)0103 physical sciencesimage processing [Techniques]010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesEvent Horizon TelescopePhysicsGround truthSupermassive black holetechniques: high angular resolutionAstronomy and AstrophysicsBlack hole physicsgalaxies: jetsindividual (M87) [Galaxies]Astrophysics - Astrophysics of Galaxiesblack hole physic3. Good healthOrbitInterferometryhigh angular resolution [Techniques]Space and Planetary Sciencetechniques: interferometricAstrophysics of Galaxies (astro-ph.GA)interferometric [Techniques]jets [Galaxies]Deconvolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for Astrophysics
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First M87 Event Horizon Telescope Results. VII. Polarization of the Ring

2021

Full list of authors: Akiyama, Kazunori; Algaba, Juan Carlos; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chan, Chi-kwan; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Chesler, Paul M.; Cho, Ilje; Christian, Pierre; Conway, John E.…

1663010504 meteorology & atmospheric sciences1346KinoAstrophysics - astrophysics of galaxiesAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGalaxy accretion disks01 natural sciencesAstrophysics - high energy astrophysical phenomena2033Galaxies: individual: M87 1278 1346 1769 1663 16 2033 1859 5620103 physical sciencesPolarimetrySupermassive black holes1769010303 astronomy & astrophysicsAstronomy data modeling0105 earth and related environmental sciencesVery long baseline interferometryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Active galactic nucleiGalaxies: individual: M871278F510ChatterjeeAstronomy and AstrophysicsCreative commons16562Low-luminosity active galactic nuclei13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Fish <Actinopterygii>Radio interferometryHumanities1859
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Young, active radio stars in the AB Doradus moving group

2017

Context. Precise determination of stellar masses is necessary to test the validity of pre-main-sequence (PMS) stellar evolutionary models, whose predictions are in disagreement with measurements for masses below 1.2 M. To improve such a test, and based on our previous studies, we selected the AB Doradus moving group (AB Dor-MG) as the best-suited association on which to apply radio-based high-precision astrometric techniques to study binary systems. Aims. We seek to determine precise estimates of the masses of a set of stars belonging to the AB Dor-MG using radio and infrared observations. Methods. We observed in phase-reference mode with the Very Large Array (VLA) at 5 GHz and with the Eur…

European VLBI NetworkInfraredFOS: Physical sciencesContext (language use)Astrophysics01 natural sciencesRadio continuum: generalObservatorypre-main sequence [Stars]0103 physical sciencesBinaries: general010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsOrbital elementsgeneral [Binaries]010308 nuclear & particles physicsgeneral [Radio continuum]Astronomy and AstrophysicsAstrometryCoronaStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceStars: pre-main sequenceAB Doradus moving group
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First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

2019

We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μas, with characteristic sensitivity limits of ~1 mJy on baselines to ALMA and ~10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, …

010504 meteorology & atmospheric sciencesgalaxies: jetRadio galaxyAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies: individualGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgalaxies: individual: M8701 natural sciencesSubmillimeter ArrayGeneral Relativity and Quantum CosmologyTechniques: high angular resolutionindividual (M87 3C279) [Galaxies]0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics0105 earth and related environmental sciencesRemote sensingPhysicsEvent Horizon TelescopeSupermassive black hole3C279Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasarBlack hole physicsblack hole physicAstrophysics - Astrophysics of Galaxies3. Good healthhigh angular resolution [Techniques]InterferometryAmplitudeSpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]jets [Galaxies]Astrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Galaxies: individual (M87 3C279)Radio wave
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Radio Emission from Binary Stars in the AB Doradus Moving Group

2015

AbstractPrecise determination of dynamical masses of pre-main-sequence stars is essential for calibrating stellar evolution models, that are widely used to derive theoretical masses of young low-mass objects. We have determined the individual masses of the pair AB Dor Ba/Bb using Australian Long Baseline Array observations and archive infrared data, as part of a larger program directed to monitor binary systems in the AB Doradus moving group. We have detected, for the first time, compact radio emission from both stars. This has allowed us to determine the orbital parameters of both the relative and absolute orbits and, consequently, their individual dynamical masses: 0.28±0.05 M⊙ and 0.25±0…

Orbital elementsPhysicsStarsSpace and Planetary ScienceInfraredBinary starBinary numberAstronomyAstronomy and AstrophysicsAstrophysicsStellar evolutionAB Doradus moving groupProceedings of the International Astronomical Union
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First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon

2021

Full list of authors: Akiyama, Kazunori; Algaba, Juan Carlos; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chan, Chi-kwan; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Chesler, Paul M.; Cho, Ilje; Christian, Pierre; Conway, John E.…

AccretionKinoAstrophysics - astrophysics of galaxiesAstrophysics::High Energy Astrophysical PhenomenaAstronomy19641347FOS: Physical sciences479Astrophysics::Cosmology and Extragalactic AstrophysicsF500870126101 natural sciences7. Clean energyAstrophysics - high energy astrophysical phenomena994MagnetohydrodynamicsRelativistic jets 14 162 479 870 886 994 1964 1261 1278 1335 1347 13900103 physical sciencesJetsPolarimetryRadiative transferPlasma astrophysicsRadio jets010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics162High Energy Astrophysical Phenomena (astro-ph.HE)Physics1278Event horizons1335010308 nuclear & particles physicsBlack holesChatterjee14886Astronomy and AstrophysicsCreative commons139013. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Magnetic fieldsKerr black holesFish <Actinopterygii>Relativistic jetsHumanities
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First M87 Event Horizon Telescope Results. I. the Shadow of the Supermassive Black Hole

2019

When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon. To image and study this phenomenon, we have assembled the Event Horizon Telescope, a global very long baseline interferometry array observing at a wavelength of 1.3 mm. This allows us to reconstruct event-horizon-scale images of the supermassive black hole candidate in the center of the giant elliptical galaxy M87. We have resolved the central compact radio source as an asymmetric bright emission ring with a diameter of 42 ± 3 μas, which is circular and encompasses a central depression in brightness with a flux rati…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonAstronomyblack hole physicsjets [galaxies]galaxies: individualAstrophysicshigh-resolution7. Clean energy01 natural sciencesPhoton sphereGeneral Relativity and Quantum Cosmologyaccretionsagittarius-a-asterisk010303 astronomy & astrophysicsgalactic-centerHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsradio-sourcesaccretion disksGalactic Centergrmhd simulations3. Good healthenergy-distributionsactive [galaxies]AnatomyAstrophysics - High Energy Astrophysical PhenomenaActive galactic nucleusAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgalaxies: individual: M87galaxies: individual (M87)Cell and Developmental BiologyGeneral Relativity and Quantum Cosmology0103 physical sciences(M87)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeghz vlbi observationsfaraday-rotationAstronomy and Astrophysicsgalaxies: jetsAstrophysics - Astrophysics of GalaxiesBlack holeRotating black holeSpace and Planetary SciencegravitationAstrophysics of Galaxies (astro-ph.GA)advection-dominated accretion[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]ionized-gas
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Monitoring the Morphology of M87* in 2009-2017 with the Event Horizon Telescope

2020

All authors: Wielgus, Maciek; Akiyama, Kazunori; Blackburn, Lindy; Chan, Chi-kwan; Dexter, Jason; Doeleman, Sheperd S.; Fish, Vincent L.; Issaoun, Sara; Johnson, Michael D.; Krichbaum, Thomas P.; Lu, Ru-Sen; Pesce, Dominic W.; Wong, George N.; Bower, Geoffrey C.; Broderick, Avery E.; Chael, Andrew; Chatterjee, Koushik; Gammie, Charles F.; Georgiev, Boris; Hada, Kazuhiro Loinard, Laurent; Markoff, Sera; Marrone, Daniel P.; Plambeck, Richard; Weintroub, Jonathan; Dexter, Matthew; MacMahon, David H. E.; Wright, Melvyn; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barausse, Enrico; Barrett, John; Bintley, Dan; Boland, Wilf…

Brightness1663Active galactic nucleus010504 meteorology & atmospheric sciences1346Event horizonAstronomyAstrophysics::High Energy Astrophysical PhenomenaGalaxy accretion disksFOS: Physical sciencesAstrophysicsF500Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences5752033Settore FIS/05 - Astronomia e AstrofisicaSupermassive black holes0103 physical sciencesVery-long-baseline interferometryAstronomy Astrophysics and Cosmology1769010303 astronomy & astrophysicsComputer Vision and Robotics (Autonomous Systems)Astronomy data modelingVery long baseline interferometry0105 earth and related environmental sciences162Black holes; Galaxy accretion disks; Galaxy accretion; Supermassive black holes; Active galactic nuclei; Low-luminosity active galactic nuclei; Very long baseline interferometry; Astronomy data modeling; Radio interferometryEvent Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Active galactic nucleiSupermassive black holeBlack holesAstronomy and Astrophysics16Galaxy accretion562Position angleGalaxyLow-luminosity active galactic nucleiMedical Image ProcessingSpace and Planetary ScienceRadio interferometryAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]1859
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The milliarcsecond-scale radio structure of AB Dor A

2020

Context: The fast rotator, pre-main sequence star AB Dor A is a strong and persistent radio emitter. The extraordinary coronal flaring activity is thought to be the origin of compact radio emission and other associated phenomena as large slingshot prominences. Aim: We aim to investigate the radio emission mechanism and the milliarcsecond radio structure around AB Dor A. Methods: We performed phase-referenced VLBI observations at 22.3 GHz, 8.4 GHz, and 1.4 GHz over more than one decade using the Australian VLBI array. Results: Our 8.4 GHz images show a double core-halo morphology, similar at all epochs, with emission extending at heights between 5 and 18 stellar radii. Furthermore, the seque…

PhysicsScale (ratio)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaStructure (category theory)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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A large rotating structure around AB Doradus A at VLBI scale

2019

AbstractWe report the results of three VLBI observations of the pre-main-sequence star AB Doradus A at 8.4 GHz. With almost three years between consecutive observations, we found a complex structure at the expected position of this star for all epochs. Maps at epochs 2007 and 2010 show a double core-halo morphology while the 2013 map reveals three emission peaks with separations between 5 and 18 stellar radii. Furthermore, all maps show a clear variation of the source structure within the observing time. We consider a number of hypothesis in order to explain such observations, mainly: magnetic reconnection in loops on the polar cap, a more general loop scenario and a close companion to AB D…

PhysicsSource structure010308 nuclear & particles physicsStructure (category theory)Astronomy and AstrophysicsScale (descriptive set theory)Magnetic reconnectionAstrophysicsStar (graph theory)01 natural sciencesSpace and Planetary SciencePosition (vector)0103 physical sciencesVery-long-baseline interferometryVariation (astronomy)010303 astronomy & astrophysicsProceedings of the International Astronomical Union
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First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole

2019

We present measurements of the properties of the central radio source in M87 using Event Horizon Telescope data obtained during the 2017 campaign. We develop and fit geometric crescent models (asymmetric rings with interior brightness depressions) using two independent sampling algorithms that consider distinct representations of the visibility data. We show that the crescent family of models is statistically preferred over other comparably complex geometric models that we explore. We calibrate the geometric model parameters using general relativistic magnetohydrodynamic (GRMHD) models of the emission region and estimate physical properties of the source. We further fit images generated fro…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonGeneral relativityAstronomyAstrophysics::High Energy Astrophysical Phenomenablack hole physicsFOS: Physical sciencesgalaxies: individualAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)GravitationGeneral Relativity and Quantum Cosmology0103 physical sciences(M87)010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsEvent Horizon TelescopeHigh Energy Astrophysical Phenomena (astro-ph.HE)high angular resolution [techniques]techniques: high angular resolutionAstronomy and Astrophysicsblack hole physicAstrophysics - Astrophysics of GalaxiesGalaxyinterferometric [techniques]Black holeRotating black holeSpace and Planetary Sciencegravitationtechniques: interferometricAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaSchwarzschild radius
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Verification of Radiative Transfer Schemes for the EHT

2020

Authors: Gold, Roman; Broderick, Avery E.; Younsi, Ziri; Fromm, Christian M.; Gammie, Charles F.; Mościbrodzka, Monika; Pu, Hung-Yi; Bronzwaer, Thomas; Davelaar, Jordy; Dexter, Jason; Ball, David; Chan, Chi-kwan; Kawashima, Tomohisa; Mizuno, Yosuke; Ripperda, Bart; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca Baczko, Anne-Kathrin; Baloković, Mislav; Barrett, John; Bintley, Dan; Blackburn, Lindy; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broguiere, Dominique; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chatterjee, Koushik; Chatterjee, Shami; Chen, Ming-T…

1388010504 meteorology & atmospheric sciencesGeodesicGeneral relativityEvent horizonAstronomyAstrophysics::High Energy Astrophysical PhenomenaKerr metric15947901 natural sciencesRelativistic disks739Relativity0103 physical sciencesRadiative transferRadiative transfer1769Radio astronomy010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesVery long baseline interferometryPhysicsEvent Horizon Telescope[PHYS]Physics [physics]Supermassive black holeEvent horizons1335Astronomy and AstrophysicsBlack hole physics1393641Computational physicsBlack holeGeneral relativitySpace and Planetary Science1338[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]High energy astrophysics
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Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution

2020

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Open Access funding provided by Max Planck Society.--All authors: Kim, Jae-Young; Krichbaum, Thomas P.; Broderick, Avery E.; Wielgus, Maciek; Blackburn, Lindy; Gómez, José L.; Johnson, Michael D.; Bouman, Katherine L.; Chael, Andrew; Akiyama, Kazunori; Jorstad, Svetlana; Marscher, Alan P.; Issaoun, Sara; Janssen, Michael; Chan, Chi-kwan; Savolainen, Tuomas; Pesce, Dominic W.; Özel, Feryal; Alberdi, Antxon; Alef, Walt…

ACTIVE GALACTIC NUCLEIBrightnessActive galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaAstronomygalaxies: activeAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSubmillimeter ArrayFLOWSSCALE CIRCULAR-POLARIZATION0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsEvent Horizon Telescope[PHYS]Physics [physics]Jet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsFLAREgalaxies: jetsindividual: 3C 279 [Galaxies]LONGVARIABILITYgalaxies: individual: 3C 279GAMMA-RAYQUASARS13. Climate actionSpace and Planetary Sciencetechniques: interferometricBrightness temperatureACCRETION DISKSinterferometric [Techniques]jets [Galaxies]RELATIVISTIC JETS[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & astrophysics
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Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign

2021

Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; …

Accretion010504 meteorology & atmospheric sciencesAstronomyFluxAstrophysics7. Clean energy01 natural sciencesActive galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; Accretion; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HERadio coreAccretion (meteorology)PhysicsAstrophysical black holes520 Astronomie und zugeordnete WissenschaftenActive galactic nuclei ; Radio cores ; Low-luminosity ; active galactic nuclei ; High energy astrophysics ; Astrophysical black holes ; AccretionAstrophysical black holeLow-luminosity active galactic nucleiastro-ph.COAstrophysics - High Energy Astrophysical PhenomenaAccretion; Active galactic nuclei; Astrophysical black holes; High energy astrophysics; Low-luminosity active galactic nuclei; Radio coresHigh energy astrophysicsRadio coresAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusHigh-energy astronomyastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesF500Astrophysics::Cosmology and Extragalactic AstrophysicsHigh energy astrophysic0103 physical sciencesVery-long-baseline interferometryddc:530Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeActive galactic nucleiAstronomy and Astrophysics530 PhysikAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ddc:520Active galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; AccretionHESS - Abteilung Hinton[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The Polarized Image of a Synchrotron-emitting Ring of Gas Orbiting a Black Hole

2021

Full list of authors: Narayan, Ramesh; Palumbo, Daniel C. M.; Johnson, Michael D.; Gelles, Zachary; Himwich, Elizabeth; Chang, Dominic O.; Ricarte, Angelo; Dexter, Jason; Gammie, Charles F.; Chael, Andrew A.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Algaba, Juan Carlos; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Domini…

AstrofísicaCamps magnèticsAccretion010504 meteorology & atmospheric sciencesAstronomyAstrophysics::High Energy Astrophysical PhenomenaStrong gravitational lensingSynchrotron radiationFOS: Physical sciencesF50001 natural sciencesAstrophysics - high energy astrophysical phenomena994General Relativity and Quantum Cosmology0103 physical sciencesPolarimetrySchwarzschild metric010303 astronomy & astrophysics0105 earth and related environmental sciences162astro-ph.HEEvent Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)1278Accretion (meteorology)Black holes14Astronomy and AstrophysicsPolarization (waves)Computational physicsMagnetic fieldBlack holeSpace and Planetary ScienceMagnetic fields14 162 1278 994
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The AB Doradus system revisited: The dynamical mass of AB Dor A/C

2017

We report new radio interferometric observations of the quadruple pre-main-sequence (PMS) system ABD oradus. From these observations, combined with existing VLT near-infrared relative astrometry, we have refined the estimates of the dynamical masses of the system. In particular, we find component masses of 0.86 ± 0.09M⊙ and 0.090 ± 0.003M⊙ for ABD or A and ABD or C, respectively. These dynamical masses, coupled with temperatures and luminosities, allow for comparison with theoretical stellar models. The case of ABDorC, in terms of calibration of evolutionary models of low-mass young stars has been widely reported in previous studies. In this contribution, we compare the measured properties …

Physics[PHYS]Physics [physics]010308 nuclear & particles physicsCalibration (statistics)Component (thermodynamics)AstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrometryAstrophysics01 natural sciencesStarsInterferometry13. Climate actionSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUS
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Event Horizon Telescope observations of the jet launching and collimation in Centaurus A

2021

Full list of authors: Janssen, Michael; Falcke, Heino; Kadler, Matthias; Ros, Eduardo; Wielgus, Maciek; Akiyama, Kazunori; Baloković, Mislav; Blackburn, Lindy; Bouman, Katherine L.; Chael, Andrew; Chan, Chi-kwan; Chatterjee, Koushik; Davelaar, Jordy; Edwards, Philip G.; Fromm, Christian M.; Gómez, José L.; Goddi, Ciriaco; Issaoun, Sara; Johnson, Michael D.; Kim, Junhan; Koay, Jun Yi; Krichbaum, Thomas P.; Liu, Jun; Liuzzo, Elisabetta; Markoff, Sera; Markowitz, Alex; Marrone, Daniel P.; Mizuno, Yosuke; Müller, Cornelia; Ni, Chunchong; Pesce, Dominic W.; Ramakrishnan, Venkatessh; Roelofs, Freek; Rygl, Kazi L. J.; van Bemmel, Ilse; Event Horizon Telescope Collaboration.--This Open Access artic…

AstrofísicaActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesEvent horizonastro-ph.GAAstronomyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics - astrophysics of galaxiesAstrophysics - cosmology and nongalactic astrophysicsCentaurus AFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstrophysics - high energy astrophysical phenomena0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesAstronomia ObservacionsEvent Horizon TelescopePhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Supermassive black holeJet (fluid)Galactic CenterAstronomy and AstrophysicsAstrophysics of Galaxies (astro-ph.GA)astro-ph.CO
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Constraints on black-hole charges with the 2017 EHT observations of M87*

2021

Full list of authors: Kocherlakota, Prashant; Rezzolla, Luciano; Falcke, Heino; Fromm, Christian M.; Kramer, Michael; Mizuno, Yosuke; Nathanail, Antonios; Olivares, Héctor; Younsi, Ziri; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Algaba, Juan Carlos; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; …

PhysicsGravitació010308 nuclear & particles physicsAstronomyKinoAstrophysics::High Energy Astrophysical Phenomenagr-qcChatterjeeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Creative commons01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesAstronomiaFish <Actinopterygii>010306 general physicsGeneral relativity and quantum cosmologyHumanitiesPhysical Review D. Particles and Fields
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