Search results for " galactic"

showing 10 items of 140 documents

MOJAVE VII. Blazar jet acceleration

2012

We discuss acceleration measurements for a large sample of extragalactic radio jets from the Monitoring Of Jets in Active Galactic Nuclei with VLBA Experiments (MOJAVE) program, which studies the parsec-scale jet structure and kinematics of a complete, flux-density-limited sample of active galactic nuclei (AGNs). Accelerations are measured from the apparent motion of individual jet features or "components" which may represent patterns in the jet flow. We find that significant accelerations are common both parallel and perpendicular to the observed component velocities. Cone search capability for table J/ApJ/706/1253/agn (Positions for AGN sources)

interstellar mediumActive galactic nucleigalactic and extragalactic astronomyAstrophysics and AstronomyRadio sourceshigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysstellar astronomyCosmologyobservational astronomyRadio continuum emissionBL Lacertae objectsHigh Energy Physics::ExperimentRadio astronomyNatural SciencesQuasarsAstrophysics::Galaxy Astrophysics
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MOJAVE. XII. Acceleration of blazar jets

2015

We report on the acceleration properties of 329 features in 95 blazar jets from the MOJAVE Very Long Baseline Array program. Nearly half the features and three-quarters of the jets show significant changes in speed and/or direction. In general, apparent speed changes are distinctly larger than changes in direction, indicating that changes in the Lorentz factors of jet features dominate the observed speed changes rather than bends along the line of sight. Observed accelerations tend to increase the speed of features near the jet base, <~10-20pc projected, and decrease their speed at longer distances. The range of apparent speeds at a fixed distance in an individual jet can span a factor of a…

interstellar mediumActive galactic nucleigalactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsSurveysstellar astronomyCosmologyobservational astronomyRadio continuum emissionRadio astronomyNatural SciencesQuasars
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MOJAVE. XIII. New 15GHz observations on 1994-2013

2017

We present 1625 new 15GHz (2cm) VLBA images of 295 jets associated with active galactic nuclei (AGNs) from the MOJAVE and 2cm VLBA surveys, spanning observations between 1994 August 31 and 2013 August 20. For 274 AGNs with at least 5 VLBA epochs, we have analyzed the kinematics of 961 individual bright features in their parsec-scale jets. A total of 122 of these jets have not been previously analyzed by the MOJAVE program. In the case of 451 jet features that had at least 10 epochs, we also examined their kinematics for possible accelerations. At least half of the well-sampled features have non-radial and/or accelerating trajectories, indicating that non-ballistic motion is common in AGN je…

interstellar mediumgalactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsRadio sourcesAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRedshiftedstellar astronomyCosmologyobservational astronomyRadio continuum emissionBL Lacertae objectsProper motionsRadio astronomyNatural SciencesQuasarsAstrophysics::Galaxy Astrophysics
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HAWC Gamma-Ray survey, AGNs at TeV photon energies

2022

The High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory continuously detects TeV photons and particles within its large field of view, accumulating every day a deeper exposure of two-thirds of the sky. We analyzed 1523days of HAWC live data acquired over four and a half years, in a follow-up analysis of 138 nearby (z<0.3) active galactic nuclei from the Third Catalog of Hard Fermi-LAT sources culminating within 40{deg} of the zenith at Sierra Negra, the HAWC site. This search for persistent TeV emission used a maximum- likelihood analysis assuming intrinsic power-law spectra attenuated by pair production of gamma-ray photons with the extragalactic background light. HAWC clearly detec…

observational astronomyActive galactic nucleigalactic and extragalactic astronomyAstrophysics and AstronomyGamma-ray astronomyhigh energy astrophysicsPhysicsGamma ray astronomySurveysNatural Sciences
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TANAMI II. Additional sources

2018

TANAMI is a multiwavelength program monitoring active galactic nuclei (AGN) south of -30{deg} declination including high-resolution Very Long Baseline Interferometry (VLBI) imaging, radio, optical/UV, X-ray and {gamma}-ray studies. We have previously published first-epoch 8.4GHz VLBI images of the parsec-scale structure of the initial sample. In this paper, we present images of 39 additional sources. The full sample comprises most of the radio- and {gamma}-ray brightest AGN in the southern quarter of the sky, overlapping with the region from which high-energy (>100TeV) neutrino events have been found. We characterize the parsec-scale radio properties of the jets and compare with the quasi-s…

observational astronomyActive galactic nucleigalactic and extragalactic astronomyAstrophysics and Astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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TANAMI monitoring of Centaurus A.

2015

Centaurus A (Cen A) is the closest radio-loud active galactic nucleus. Very Long Baseline Interferometry (VLBI) enables us to study the spectral and kinematic behavior of the radio jet-counterjet system on milliarcsecond scales, providing essential information for jet emission and propagation models. In the framework of the TANAMI monitoring, we investigate the kinematics and complex structure of Cen A on subparsec scales. We have been studying the evolution of the central parsec jet structure of Cen A for over 3.5-years. The proper motion analysis of individual jet components allows us to constrain jet formation and propagation and to test the proposed correlation of increased high-energy …

observational astronomygalactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsRadio galaxiesAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesGalaxiesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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The gNLS1 galaxy PKS 2004-447. VLBI images

2016

Gamma-ray-detected radio-loud narrow-line Seyfert 1 (g-NLS1) galaxies constitute a small but interesting sample of the g-ray-loud AGN. The radio-loudest g-NLS1 known, PKS 2004-447, is located in the southern hemisphere and is monitored in the radio regime by the multiwavelength monitoring programme TANAMI. We aim for the first detailed study of the radio morphology and long-term radio spectral evolution of PKS 2004-447, which are essential for understanding the diversity of the radio properties of g-NLS1s. The TANAMI VLBI monitoring program uses the Australian Long Baseline Array (LBA) and telescopes in Antarctica, Chile, New Zealand, and South Africa to monitor the jets of radio-loud activ…

observational astronomygalactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsRadio galaxiesAstrophysics::Cosmology and Extragalactic AstrophysicsNatural SciencesGalaxiesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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Sample of weak blazars at mas resolution

2015

We started a follow-up investigation of the "Deep X-ray Radio Blazar Survey" objects with declination >-10{deg} to better understand the blazar phenomenon. We undertook a survey with the European Very Long Baseline Interferometry Network at 5GHz to make the first images of a complete sample of weak blazars, aiming at a follow-up comparison between high- and low-power samples of blazars. We observed 87 sources with the EVN at 5GHz during the period October 2009 to May 2013. The observations were correlated at the Max-Planck-Institut fuer Radioastronomie and at the Joint Institute for VLBI in Europe. The correlator output was analysed using both the AIPS and DIFMAP software packages. All of t…

observational astronomygalactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsRadio sourcesPhysicsBL Lacertae objectsRadio astronomyNatural Sciencesstellar astronomyQuasarsCosmology
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Constructing a Transmedia Universe : The Case of Battlestar Galactica

2021

In this article, we define a ‘transmedia universe’ as encompassing the complexity of transmedia storytelling, production and consumption. In doing so, we use the popular science fiction television series Battlestar Galactica as a case study, including both the original and reimagined versions of the series and their various intramedia and transmedia, narrative and non-narrative, and diegetic and non-diegetic expansions. Moreover, we look beyond the official productions of the Battlestar Galactica franchise and include, for example, user-generated content within its transmedia universe. peerReviewed

sisältötuotantoscifipelittieteissarjatTaisteluplaneetta Galacticatransmedia universetransmediafaniustransmedia storytellingtransmedial worldBattlestar Galacticauser-generated contenttieteiskirjallisuus
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Reimagining humanity in Battlestar Galactica, Bionic Woman and V

2015

sukupuolentutkimusfeminist posthumanismBionic Woman (televisio-ohjelma)muukalaisuusfeministinen tutkimuspassing for humanerilaisuusposthumanist ethicsscience fiction televisionrepresentaatioperformativitylivable livesvierausfeminist theorytieteissarjattelevisiosarjatihmisyysgendertieteisfiktioethnicityTaisteluplaneetta Galactica (televisio-ohjelma)ihmiskuvaV (televisio-ohjelma)
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