Search results for "GALAXIES"

showing 10 items of 341 documents

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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On the carrier of inertia

2018

A change in momentum will inevitably perturb the all-embracing vacuum, whose reaction we understand as inertia. Since the vacuum's physical properties relate to light, we propose that the vacuum embodies photons, but in pairs without net electromagnetic fields. In this physical form the free space houses energy in balance with the energy of matter in the whole Universe. Likewise, we reason that a local gravitational potential is the vacuum in a local balance with energy that is bound to a body. Since a body couples to the same vacuum universally and locally, we understand that inertial and gravitational masses are identical. By the same token, we infer that gravity and electromagnetism shar…

ANOMALIESPhotonmedia_common.quotation_subjectvacuumUNIVERSEGeneral Physics and AstronomyCosmological constantPHOTONSInertia01 natural sciencesGravitationMomentumGeneral Relativity and Quantum CosmologyGravitational potentialElectromagnetism0103 physical sciences010306 general physics010303 astronomy & astrophysicsCOSMOLOGICAL CONSTANTmedia_commonPhysicsfotonitta114LEAST-ACTIONgravitaatioinertialiike115 Astronomy Space sciencelcsh:QC1-999UniverseTIMEmotion (physical phenomena)GALAXIESClassical mechanicsgravitationWAVEPRINCIPLECLUSTERSlcsh:PhysicsAIP Advances
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A parametric description of the 3D structure of the Galactic bar/bulge using the VVV survey

2017

We study the structure of the inner Milky Way using the latest data release of the Vista Variables in Via Lactea (VVV) survey. The VVV is a deep near-infrared, multi-colour photometric survey with a coverage of 300 square degrees towards the Bulge/Bar. We use Red Clump (RC) stars to produce a high-resolution dust map of the VVV's field of view. From de-reddened colour-magnitude diagrams we select Red Giant Branch stars to investigate their 3D density distribution within the central 4 kpc. We demonstrate that our best-fit parametric model of the Bulge density provides a good description of the VVV data, with a median percentage residual of 5$\%$ over the fitted region. The strongest of the o…

Absolute magnitudeInitial mass functionastro-ph.GAMilky WayFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: bulgeBulge0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsRed clumpGalaxy: structureAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLuminosity function (astronomy)Physics010308 nuclear & particles physicsGalactic CenterAstronomyAstronomy and AstrophysicsGalaxy: fundamental parametersAstrophysics - Astrophysics of GalaxiesGalaxy: centregalaxies: individual: Milky WayRed-giant branchSpace and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Detection of deuterated molecules, but not of lithium hydride, in the z = 0.89 absorber toward PKS 1830−211

2020

Deuterium and lithium are light elements of high cosmological and astrophysical importance. In this work we report the first detection of deuterated molecules and a search for lithium hydride, 7LiH, at redshift z=0.89 in the spiral galaxy intercepting the line of sight to the quasar PKS1830-211. We used ALMA to observe several submillimeter lines of ND, NH2D, and HDO, and their related isotopomers NH2, NH3, and H2^18O, in absorption against the southwest image of the quasar, allowing us to derive XD/XH abundance ratios. The absorption spectra mainly consist of two distinct narrow velocity components for which we find remarkable differences. One velocity component shows XD/XH abundances that…

Absorption spectroscopyquasarsFOS: Physical scienceschemistry.chemical_elementAstrophysics01 natural scienceschemistry.chemical_compound0103 physical sciencesISM -galaxiesgalaxiesindividual010303 astronomy & astrophysicsLine (formation)Physics[PHYS]Physics [physics]Spiral galaxy010308 nuclear & particles physicsmolecules -radio linesAstronomy and AstrophysicsQuasarAstrophysics - Astrophysics of GalaxiesRedshift3. Good healthPKS 1830−211 -galaxiesabundances -ISMDeuteriumchemistry13. Climate actionSpace and Planetary ScienceLithium hydride[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Lithium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorption lines -quasars
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QPOs expected in rotating accretion flows around a supermassive black hole

2007

It is well known that rotating inviscid accretion flows with adequate injection parameters around black holes could form shock waves close to the black holes, after the flow passes through the outer sonic point and can be virtually stopped by the centrifugal force. We numerically examine such shock waves in 2D accretion flows with 10−5 to 106 Eddington critical accretion rates around a supermassive black hole with 106 M. As the results, the luminosities show QPO phenomena with modulations of a factor 2–3 and with quasi-periods of a few to several hours.

Accretion accretion disks – black hole physics – galaxies: active – hydrodynamics – radiation mechanisms: thermal – shock waves
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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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Broad-band spectral analysis of the accreting millisecond X-ray pulsar SAX J1748.9-2021

2016

We analyzed a 115 ks XMM-Newton observation and the stacking of 8 days of INTEGRAL observations, taken during the raise of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021. The source showed numerous type-I burst episodes during the XMM-Newton observation, and for this reason we studied separately the persistent and burst epochs. We described the persistent emission with a combination of two soft thermal components, a cold thermal Comptonization component (~2 keV) and an additional hard X-ray emission described by a power-law (photon index ~2.3). The continuum components can be associated with an accretion disc, the neutron star (NS) surface and a thermal Compton…

AccretionBinaries - X-rayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesIndividualAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaPulsarSAX J1748.9-2021Millisecond pulsarAccretion discs -X-ray0103 physical sciencesAccretion; Accretion discs -X-rays; Binaries - X-rays; Galaxies -X-rays; Individual; SAX J1748.9-2021; Space and Planetary Science; Astronomy and Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSolar massMillisecondAstronomyAstronomy and AstrophysicsAccretion (astrophysics)Neutron starSpace and Planetary ScienceGalaxies -X-rayEddington luminositysymbolsAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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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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X-shooter spectroscopy of young stars with disks. The TW Hydrae association as a probe of the final stages of disk accretion

2019

We investigate ongoing accretion activity in young stars in the TW Hydrae association (TWA, ~8-10 Myr), an ideal target to probe the final stages of disk accretion down to brown dwarf masses. Our sample comprises eleven TWA members with infrared excess, amounting to 85% of the total TWA population with disks, with spectral types between M0 and M9, and masses between 0.58 and 0.02 Msol. We employed homogeneous spectroscopic data from 300 to 2500 nm, obtained with X-shooter, to derive individual extinction, stellar parameters, and accretion parameters simultaneously. We then examined Balmer lines and forbidden emission lines to probe the physics of the star-disk interaction environment. We de…

AccretionOpen clusters and associations: individual: TWA010504 meteorology & atmospheric sciencesBrown dwarfFOS: Physical sciencesTechniques: spectroscopicAstrophysicsProtoplanetary diskStellar classification01 natural sciencesspectroscopic [Techniques]symbols.namesakeSettore FIS/05 - Astronomia E Astrofisicalow-mass [Stars]pre-main sequence [Stars]0103 physical sciencesStars: low-maTW HydraeQB Astronomy010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesQBEarth and Planetary Astrophysics (astro-ph.EP)PhysicsInfrared excessBalmer seriesAstronomy and AstrophysicsDASAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)StarsQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAccretion diskAstrophysics of Galaxies (astro-ph.GA)Accretion diskssymbolsStars: pre-main sequenceindividual: TWA [Open clusters and associations]Astrophysics - Earth and Planetary Astrophysics
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Jet collimation in NGC 315

2021

VizieR online Data Catalogue associated with article published in journal Astronomy &amp; Astrophysics with title 'Jet collimation in NGC 315 and other nearby AGN.' (bibcode: 2021A&amp;A...647A..67B)

Active galactic nucleiRadio sourcesAstrophysics::High Energy Astrophysical PhenomenaRadio galaxiesAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRadio astronomyGalaxiesComputer Science::Digital LibrariesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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