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Spherical subsystem of galactic radiosources

Journal Article:

Abstract

The concentration of statistically complete sampling radiosources of the Ohiof scanning with plane spectra towards the Galaxy centre has been discovered. Quantitative calculations have showed that the sources form a spheric subsystem, which is close in parameters to such old formations in the Galaxy as globular clusters and the RRLsub(YR) type stars. The luminosity of the galaxy spheric subsystem object equals 10/sup 33/ erg/sec, the total number of objects being 7000. The existence of such a subsystem explains s the anomalously by low incline of statistics lgN-lgS in HF scanning PKS (..gamma..-2700Mgz) and the Michigan University scanning (..gamma..=8000Mgz) because the sources of galaxy spheric subsystem make up a considerable share in the total number of sources, especially at high frequencies (50% of sources with a flux greater than a unit of flux per 8000Mgz). It is very probable that the given subsystem consists of the representatives of one of the following class of objects: a) heat sources - the H2H regions with T=10/sup 40/K, Nsub(e)=10/sup 3/, l=1 ps b) supermass black holes with mass M/Mo approximately 10/sup 5/.
Authors:
Gorshkov, A G; Popov, M V [1] 
  1. Moskovskij Gosudarstvennyj Univ. (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''
Publication Date:
May 01, 1975
Product Type:
Journal Article
Reference Number:
AIX-08-314239; EDB-77-115660
Resource Relation:
Journal Name: Astron. Zh.; (USSR); Journal Volume: 52:3; Other Information: 28 refs.; 5 figs.; for English translation see the journal Sov. Astron. AJ
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; COSMIC RADIO SOURCES; LUMINOSITY; SPATIAL DISTRIBUTION; BLACK HOLES; COMPARATIVE EVALUATIONS; GALAXIES; GHZ RANGE 01-100; STATISTICS; DISTRIBUTION; FREQUENCY RANGE; GHZ RANGE; MATHEMATICS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; 640103* - Astrophysics & Cosmology- Quasi-Stellar, Radio, & X-Ray Sources- (-1987)
OSTI ID:
7302688
Country of Origin:
USSR
Language:
Russian
Other Identifying Numbers:
Journal ID: CODEN: ASZHA
Submitting Site:
INIS
Size:
Pages: 538-545
Announcement Date:

Journal Article:

Citation Formats

Gorshkov, A G, and Popov, M V. Spherical subsystem of galactic radiosources. USSR: N. p., 1975. Web.
Gorshkov, A G, & Popov, M V. Spherical subsystem of galactic radiosources. USSR.
Gorshkov, A G, and Popov, M V. 1975. "Spherical subsystem of galactic radiosources." USSR.
@misc{etde_7302688,
title = {Spherical subsystem of galactic radiosources}
author = {Gorshkov, A G, and Popov, M V}
abstractNote = {The concentration of statistically complete sampling radiosources of the Ohiof scanning with plane spectra towards the Galaxy centre has been discovered. Quantitative calculations have showed that the sources form a spheric subsystem, which is close in parameters to such old formations in the Galaxy as globular clusters and the RRLsub(YR) type stars. The luminosity of the galaxy spheric subsystem object equals 10/sup 33/ erg/sec, the total number of objects being 7000. The existence of such a subsystem explains s the anomalously by low incline of statistics lgN-lgS in HF scanning PKS (..gamma..-2700Mgz) and the Michigan University scanning (..gamma..=8000Mgz) because the sources of galaxy spheric subsystem make up a considerable share in the total number of sources, especially at high frequencies (50% of sources with a flux greater than a unit of flux per 8000Mgz). It is very probable that the given subsystem consists of the representatives of one of the following class of objects: a) heat sources - the H2H regions with T=10/sup 40/K, Nsub(e)=10/sup 3/, l=1 ps b) supermass black holes with mass M/Mo approximately 10/sup 5/.}
journal = {Astron. Zh.; (USSR)}
volume = {52:3}
journal type = {AC}
place = {USSR}
year = {1975}
month = {May}
}