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On the Radio Emission of Barred Spirals
release_qfo3x4pd3nc7vpc3irbxifsf7i
by
A.T. Kalloghlian, R.A. Kandalian
Published
in Symposium - International astronomical union by Cambridge University Press (CUP).
1987 Volume 121, p489-491
Abstract
It is found that the relation between the presence of radio emission and the degree of central concentration (i.e. the Byurakan class) of spiral galaxies is valid only for barred spirals. Barred spirals are also found to have central radio sources more often than normal spirals which are generally disc radio emitters.
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