Milky Way scattering properties and intrinsic sizes of active galactic nuclei cores probed by very long baseline interferometry surveys of compact extragalactic radio sources
arXiv:1507.02459 · doi:10.1093/mnras/stv1539
Abstract
We have measured the angular sizes of radio cores of active galactic nuclei (AGN) and analyzed their sky distributions and frequency dependencies to study synchrotron opacity in AGN jets and the strength of angular broadening in the interstellar medium. We have used archival very long baseline interferometry (VLBI) data of more than 3000 compact extragalactic radio sources observed at frequencies, , from 2 to 43 GHz to measure the observed angular size of VLBI cores. We have found a significant increase in the angular sizes of the extragalactic sources seen through the Galactic plane () at 2, 5 and 8 GHz, about 1/3 of which show significant scattering. These sources are mainly detected in directions to the Galactic bar, the Cygnus region, and a region with galactic longitudes (the Fitzgerald window). The strength of interstellar scattering of the AGNs is found to correlate with the Galactic H intensity, free-electron density, and Galactic rotation measure. The dependence of scattering strengths on source redshift is insignificant, suggesting that the dominant scattering screens are located in our Galaxy. The observed angular size of Sgr A is found to be the largest among thousands of AGN observed over the sky; we discuss possible reasons of this strange result. Excluding extragalactic radio sources with significant scattering, we find that angular size of opaque cores in AGN scales typically as confirming predictions of a conical synchrotron jet model with equipartition.
9 pages, 7 figures, 5 tables, published by MNRAS; full electronic table 2 (redshifts updated) is available from ftp://cdsarc.u-strasbg.fr/pub/cats/J/MNRAS/452/4274/
References in corpus (16)
- Sub-milliarcsecond Imaging of Quasars and Active Galactic Nuclei III. Kinematics of Parsec-Scale Radio Jets
- MOJAVE: Monitoring of Jets in AGN with VLBA Experiments. V. Multi-epoch VLBA Images
- RadioAstron -- a Telescope with a Size of 300 000 km: Main Parameters and First Observational Results
- The VLBA Imaging and Polarimetry Survey at 5 GHz
- Opacity in compact extragalactic radio sources and its effect on astrophysical and astrometric studies
- The Sixth VLBA Calibrator Survey: VCS6
- The Fifth VLBA Calibrator Survey: VCS5
- Spiral structure in the outer Galactic disk. I. The Third Galactic Quadrant
- Theory and Simulations of Refractive Substructure in Resolved Scatter-Broadened Images
- Discovery of Substructure in the Scatter-Broadened Image of Sgr A*
- VERA 22 GHz fringe search survey
- Angular Broadening of Intraday Variable AGN. II. Interstellar and Intergalactic Scattering
- The intra-hour variable quasar J18193845: 13-year evolution, jet polarization structure and interstellar scattering screen properties
- Early science with Korean VLBI network: the QCAL-1 43GHz calibrator survey
- Why Do Compact Active Galactic Nuclei at High Redshift Scintillate Less?
- Scatter broadening of compact radio sources by the ionized intergalactic medium: Prospects for detection with Space VLBI and the SKA
Cited by in corpus (48)
- MOJAVE XIII. Parsec-Scale AGN Jet Kinematics Analysis Based on 19 years of VLBA Observations at 15 GHz
- MOJAVE - XIV. Shapes and opening angles of AGN jets
- Probing the innermost regions of AGN jets and their magnetic fields with RadioAstron. I. Imaging BL Lacertae at 21 microarcsecond resolution
- Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to
- Significant core shift variability in parsec-scale jets of active galactic nuclei
- VLBI-Gaia offsets favor parsec-scale jet direction in Active Galactic Nuclei
- Measuring the speed of light with ultra-compact radio quasars
- The distance sum rule from strong lensing systems and quasars - test of cosmic curvature and beyond
- Measurements of the Hubble constant and cosmic curvature with quasars: ultra-compact radio structure and strong gravitational lensing
- The Radio Fundamental Catalogue. I. Astrometry
- Observational consequences of optical band milliarcsecond-scale structure in active galactic nuclei discovered by Gaia
- PSR B0329+54: Substructure in the scatter-broadened image discovered with RadioAstron on baselines up to 330,000 km
- A new test of gravity with the cosmological standard rulers in radio quasars
- Testing the Etherington's distance duality relation at higher redshifts: the combination of radio quasars and gravitational waves
- Scintillation timescale measurement of the highly active FRB20201124A
- A decade of joint MOJAVE-Fermi AGN monitoring: localisation of the gamma-ray emission region
- Revising the Hubble constant, spatial curvature and dark energy dynamics with the latest observations of quasars
- Cosmological investigation of multi-frequency VLBI observations of ultra-compact structure in radio quasars
- The extreme blazar AO 0235+164 as seen by extensive ground and space radio observations
- Resolving the decades-long transient FIRST J141918.9+394036: an orphan long gamma-ray burst or a young magnetar nebula?
- The high brightness temperature of B0529+483 revealed by RadioAstron and implications for interstellar scattering
- Direction of Parsec-Scales Jets for 9220 Active Galactic Nuclei
- Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
- Tracing Milky Way scattering by compact extragalactic radio sources
- Constraints on the location of -ray emitting region for a sample of blazars with radio core-shift measurements
- Parsec-scale properties of steep and flat spectrum extragalactic radio sources from a VLBA survey of a complete north polar cap sample
- The MASIV Survey IV: relationship between intra-day scintillation and intrinsic variability of radio AGNs
- Blazar jet evolution revealed by multi-epoch broadband radio polarimetry
- Localizing the -ray emitting region in the blazar TXS 2013+370
- Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO
- Parsec-scale properties of the peculiar gigahertz-peaked spectrum quasar 0858-279
- A single HII region model of the strong interstellar scattering towards Sgr A*
- Effelsberg Monitoring of a Sample of RadioAstron Blazars: Analysis of Intra-Day Variability
- Parabolic jet shape on parsec scales in high redshift AGN
- High-resolution imaging with the International LOFAR Telescope: Observations of the gravitational lenses MG 0751+2716 and CLASS B1600+434
- Testing and selecting cosmological models with ultra-compact radio quasars
- A method for checking high-redshift identification of radio AGNs
- Rotation Measure synthesis study and polarized properties of PSR J1745-2900 at 7 mm
- PKS 1954-388: RadioAstron Detection on 80,000 km Baselines and Multiwavelength Observations
- Parsec-scale evolution of the gigahertz-peaked spectrum quasar PKS 0858-279
- Dim cores of radio-bright AGN jets: VLBI and Gaia astrometry pinpoint different parsec-scale features
- A long-lived compact jet in the black hole X-ray binary candidate AT2019wey
- Structural and spectral properties of Galactic plane variable radio sources
- Radio and Optical Properties of the blazar PKS 1614+051 at z=3.21
- Influence of the Galactic gravitational field on the positional accuracy of extragalactic sources. II Observational appearances and detectability
- Sun-related variability in the light curves of compact radio sources. A new view on Extreme Scattering Events
- Direct VLBI Detection of Interstellar Turbulence Imprint on a Quasar: TXS 2005+403
- Heavy interstellar scattering toward the near end of the Galactic bar