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On the question of radio emission of spiral galaxies in groups of galaxies

✍ Scribed by V. H. Malumian

Publisher
John Wiley and Sons
Year
1996
Tongue
English
Weight
423 KB
Volume
317
Category
Article
ISSN
0004-6337

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✦ Synopsis

It has been shown that the radio emission properties of spiral galaxies, if the other conditions are the same, are determined rather by the presence of the close neighbours than by space density of galaxies around them. The rate of occurence of radio sources and their radio luminosities among the spiral members of groups of galaxies depend on the projected seperation between them and their nearest neighbour. The shorter this seperation the higher the probability of radio emission.

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