The bivariant luminosity function for isolated galaxy pairs

Details The bivariant luminosity function for isolated galaxy pairs The bivariant luminosity function for isolated galaxy pairs

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..441p&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, May-June 1984, p. 441-449) Soviet Astronomy (ISSN 0038-5301), vol. 28, May-June 1984, p. 258

Astronomy and Astrophysics

Astronomy

2

Astronomical Catalogs, Luminosity, Radiant Flux Density, Radio Astronomy, Radio Galaxies, Correlation Coefficients, Light Emission, Radial Velocity, Radio Emission, Statistical Distributions

Scientific paper

The radio observations of Stocke et al. (1978) on isolated galaxy pairs from the catalog of Karachentsev (1972) are analyzed using the method of Arakelyan (1984) to calculate the optical/radio bivariant luminosity functions (BLFs). The results are presented in tables and graphs and characterized statistically. The discrepancy between the BLFs of type EE pairs and those of ES/SE or SS pairs is attributed to pseudopairing in the EE pairs, and the number density of the radio pairs is found to be about 0.0004/cu Mpc, as compared to 0.004/cu Mpc for all paired galaxies.

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