Abstract
This is a brief review of investigations of AGNs by the interplanetary scintillation method made in Pushchino Radio Astronomy Observatory.
Similar content being viewed by others
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.
Artyukh, V.S.: 1990, Interplanetary Scintillation Observations of Meter-Wavelength Radio Emission from Galaxies, in: N.G. Basov (ed.), Proceedings of the Lebedev Physics Institute, Academy of Sciences of the USSR, 189, pp. 289–309. Nova Science Publishers New York/Budapest.
Artyukh, V.S.: 1997, The Influence of Scattering of Radio Emission on Scintillating Radio Source Counts, Astron. Rep. 41, 160–162.
Artyukh, V.S.: 2000, A Search of Large-Scale Inhomogeneities in a Compact Radio Source Distribution, Astron. Rep. 44, 349–352.
Artyukh, V.S. and Chernikov, P.A.: 2001, Synchrotron Spectra of Inhomogeneous Radio Sources, Astron. Rep. 45, 16–25.
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.
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.
Artyukh, V.S. and Ogannisian, M.A.: 1993, The Investigation of the Perceus Cluster of Galaxies at 102 MHz, Astronomicheskii J. 70, 443–450.
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.
Artyukh, V.S. and Shishova, T.D.: 1987, About the Resolution of the IPS Method, Radiofisika 30, 1396.
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.
Artyukh, V.S. and Tyul'bashev, S.A. 1998, The Cosmological Evolution of Quasars with Steep Spectra, Astron. Rep. 42, 576–586.
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.
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.
Chandrasekhar, S.: 1952, A Statistical Basis for the Theory of Stellar Scintillation, MNRAS 112, 475–484.
Hewish, A., Scott, P.F. and Wills, D.: 1964, Interplanetary Scintillation of Small Diameter Radio Sources, Nature 203, 1214–1217.
Shishov, V.I. and Shishova, T.D.: 1978, Influence of Source Sizes on the Spectra of Interplanetary Scintillations, Soviet Astron. 22, 235–239.
Tyul'bashev, S.A. and Chernikov, P.A.: 2000, Physical Conditions in Steep Spectrum Compact Radio Sources, Astron. Rep. 44, 286–299.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Artyukh, V.S. Investigations of AGNs by the interplanetary scintillation method. Astrophysics and Space Science 278, 185–188 (2001). https://doi.org/10.1023/A:1013154728238
Issue Date:
DOI: https://doi.org/10.1023/A:1013154728238