Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-27T21:31:59.656Z Has data issue: false hasContentIssue false
  • English
  • Français

Investigations of AGNS by the Interplanetary Scintillation Method

Published online by Cambridge University Press:  12 April 2016

Vadim S. Artyukh
Vadim S. Artyukh*
Affiliation:
Pushchino Radio Astronomy Observatory of the Lebedev Physical Institute RAS, Leninskii pr. 53, 117924, Moscow, Russia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

This is a brief review of investigations of AGNs by the interplanetary scintillation method made in Pushchino Radio Astronomy Observatory.

Keywords

compact radio sourceactive galactic nucleusphysical conditionscosmologyinterplanetary scintillations
Type
Chapter Four Extreme Scattering Events, Distribution of Material and IPS
Information
International Astronomical Union Colloquium , Volume 182: Sources and Scintillations: Refraction and Scattering in Radio Astronomy , 2001 , pp. 185 - 188
Copyright
Copyright © Kluwer 2001

References

Artyukh, V.S.: 1987, The Radio Spectra of Scintillating Sources, and the Morphological Type of the Active Host galaxies, Soviet Astronomy Letters 13, 108–112.Google Scholar
Artyukh, V.S.: 1990, Interplanetary Scintillation Observations of Meter-Wavelength Radio Emission from Galaxies, in: Basov, N.G. (ed.), Proceedings of the Lebedev Physics Institute, Academy of Sciences of the USSR, 189, pp. 289–309. Nova Science Publishers New York/Budapest.Google Scholar
Artyukh, V.S.: 1997, The Influence of Scattering of Radio Emission on Scintillating Radio Source Counts, Astron. Rep. 41, 160–162.Google Scholar
Artyukh, V.S.: 2000, A Search of Large-Scale Inhomogeneities in a Compact Radio Source Distribution, Astron. Rep. 44, 349–352.CrossRefGoogle Scholar
Artyukh, V.S. and Chernikov, P.A.: 2001, Synchrotron Spectra of Inhomogcneous Radio Sources, Astron. Rep. 45, 16–25.CrossRefGoogle Scholar
Artyukh, V.S. and Ogannisian, M.A.: 1988(a), The Observation of the Giant Radio Galaxies 3C 236 and DA 240 at 102 MHz, Pis’ma v Astronomy Journal 14, 706–712.Google Scholar
Artyukh, V.S. and Ogannisian, M.A.: 1988(b). A Large-Scale Void in the Distribution of Compact Radio Sources, Soviet Astronomy Letters 14, 377–378.Google Scholar
Artyukh, V.S. and Ogannisian, M.A.: 1993, The Investigation of the Pcrceus Cluster of Galaxies at 102 MHz, Astronomicheskii J. 70, 443–450.Google Scholar
Artyukh, V.S., Ogannisian, M.A. and Tyul’bashev, S.A.: 1994, Observations of the Radio Galaxies NGC 315 and 3C 219 at 102 MHz, Pis’ma v Astron. J. 20, 178–183.Google Scholar
Artyukh, V.S. and Shishova, T.D.: 1987, About the Resolution of the IPS Method, Radiofisika 30, 1396.Google Scholar
Artyukh, V.S. and Tyul’bashev, S.A.: 1996, The Cosmological Evolution of Compact Radio Sources from 102 MHz Observations, Astron. Rep. 40, 661–668.Google Scholar
Artyukh, V.S. and Tyul’bashev, S.A. 1998, The Cosmological Evolution of Quasars with Steep Spectra, Astron. Rep. 42, 576–586.Google Scholar
Artyukh, V.S., Tyul’bashev, S.A. and Chernikov, P.A.: 1999, Investigations of Compact Steep-Spectrum Radio Sources Using 102 MHz Interplanetary Scintillation Observations, Astron. Rep. 43, 1–12.Google Scholar
Artyukh, V.S., Tyul’bashev, S.A. and Isaev, E.A.: 1998, The Cosmological Evolution of Compact Radio Sources from 102 MHz Observations, Astron. Rep. 42, 283–292.Google Scholar
Chandrasekhar, S.: 1952, A Statistical Basis for the Theory of Stellar Scintillation, MNRAS 112, 475–484.Google Scholar
Hewish, A., Scott, P.F. and Wills, D.: 1964, Interplanetary Scintillation of Small Diameter Radio Sources, Nature 203, 1214–1217.CrossRefGoogle Scholar
Shishov, V.I. and Shishova, T.D.: 1978, Influence of Source Sizes on the Spectra of Interplanetary Scintillations, Soviet Astron. 22, 235–239.Google Scholar
Tyul’bashev, S.A. and Chernikov, P.A.: 2000, Physical Conditions in Steep Spectrum Compact Radio Sources, Astron. Rep. 44, 286–299.Google Scholar