Search Results - "Arshakian, Tigran G"
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1
Optimum frequency band for radio polarization observations
Published in Monthly notices of the Royal Astronomical Society (21-12-2011)Get full text
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2
Optimum frequency band for radio polarization observations
Published in Monthly notices of the Royal Astronomical Society (21-12-2011)“…Polarized radio synchrotron emission from interstellar, intracluster and intergalactic magnetic fields is affected by frequency-dependent Faraday…”
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3
Optimum frequency band for radio polarization observations: Optimum frequency band for radio observations
Published in Monthly notices of the Royal Astronomical Society (21-12-2011)Get full text
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4
The central pc-scale region in blazars: insights from multi-band observations
Published 11-01-2014“…The empirical relations in the black hole-accretion disk-relativistic jet system and physical processes behind these relations are still poorly understood,…”
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5
Optimum frequency band for radio polarisation observations
Published 11-08-2011“…Polarised radio synchrotron emission from interstellar, intracluster and intergalactic magnetic fields is affected by frequency-dependent Faraday…”
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6
Exploring weak magnetic fields with LOFAR and SKA
Published 17-04-2009“…Regular magnetic field structures can be derived from the Faraday rotation measures (RM) of polarized background sources observable at 1.4 GHz with the SKA. At…”
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7
The link between ejection of a jet component and characteristics of variable continuum emission in the active galaxy 3C 390.3
Published 21-11-2006“…PoSMQW6:029,2006 We study the correlations between the jet ejection event and changes in the continuum emission of the radio-loud galaxy 3C 390.3, using the…”
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8
Correlations between radio emission of the parsec-scale jet and optical nuclear emission of host AGN
Published 11-04-2011“…We study the relation between the VLBA (Very Long Baseline Array) radio emission at 15 GHz and the optical nuclear emission at 5100 A for a sample of 233…”
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Optical Spectroscopic ATLAS of the MOJAVE/2cm AGN Sample (1)
Published 18-07-2011“…We present an optical spectroscopic atlas at intermediate resolution (8-15A) for 123 core-dominated radio-loud active galactic nuclei with relativistic jets,…”
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Testing the cosmological evolution of magnetic fields in galaxies with the SKA
Published 16-12-2008“…We investigate the cosmological evolution of large- and small-scale magnetic fields in galaxies at high redshifts. Results from simulations of hierarchical…”
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Evolution of magnetic fields in galaxies and future observational tests with the Square Kilometre Array
Published 18-11-2008“…Aims. We investigate the cosmological evolution of large- and small-scale magnetic fields in galaxies in the light of present models of formation and evolution…”
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Evolution of magnetic fields in galaxies in the frame of hierarchical structure formation cosmology: future tests with the SKA
Published 16-09-2009“…Results from simulations of hierarchical structure formation cosmology provide a tool to develop an evolutionary model of regular magnetic fields coupled to…”
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13
Small-scale dynamo action during the formation of the first stars and galaxies. I. The ideal MHD limit
Published 23-08-2010“…We explore the amplification of magnetic seed fields during the formation of the first stars and galaxies. During gravitational collapse, turbulence is created…”
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Magnetic field structures of galaxies derived from analysis of Faraday rotation measures, and perspectives for the SKA
Published 21-01-2008“…The forthcoming new-generation radio telescope SKA (Square Kilometre Array) and its precursors will provide a rapidly growing number of polarized radio…”
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15
The source of variable optical emission is localized in the jet of the radio galaxy 3C 390.3
Published 01-02-2006“…We present observational evidence for the link between variability of the radio emission of the relativistic jet and optical continuum emission in the radio…”
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An asymmetric relativistic model for classical double radio sources
Published 20-05-1999“…An asymmetric relativistic model for FRII radio sources is described which takes account of both relativistic effects and intrinsic/environmental asymmetries…”
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17
Observational evidence for the link between the variable optical continuum and the jet of a radio-loud galaxy 3C 390.3
Published 15-12-2005“…The ``central engine'' of AGN is thought to be powered by accretion on a central nucleus believed to be a super-massive black hole. The localization and exact…”
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