Radio emission of spiral galaxies in groups of galaxies

Details Radio emission of spiral galaxies in groups of galaxies Radio emission of spiral galaxies in groups of galaxies

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....26..311m&link_type=abstract

(Astrofizika, vol. 26, Mar.-Apr. 1987, p. 311-319) Astrophysics (ISSN 0571-7132), vol. 26, no. 2, Sept. 1987, p. 190-195. Transl

Astronomy and Astrophysics

Astrophysics

5

Galactic Radiation, Radio Emission, Spiral Galaxies, Brightness, Data Sampling, Galactic Clusters

Scientific paper

It is shown that spiral galaxies that are members of groups of galaxies have radio luminosities that are less than those of spiral members of isolated binary systems but greater than those of isolated single spirals. This is true both for the brightest members of groups as well as for fainter members. Among the brightest spiral members of groups the frequency for finding radio emission is not lower than in spiral binary systems and is appreciably higher than for isolated spiral galaxies. The conclusion drawn earlier that the brightest galaxies in groups of galaxies play an active role is also confirmed.

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