Barred galaxies. IV. Comparative statistics on SB and SA galaxies in the radio and x-ray ranges |
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Authors: | R A Kandalian A T Kalloghlian |
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Institution: | (1) V. A. Ambartsumian Astrophysical Observatory, Byurakan, Armenia |
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Abstract: | The radio and xray properties of spiral galaxies with and without a bar are discussed on the basis of complete samples that
we have compiled. The two types of spirals are shown not to differ from one another in emission power in the two indicated
ranges. In the case of SB galaxies, the luminosities in the IR, radio, and xray ranges are closely related. The spectral indices
of SB and SA galaxies in the 1.4–5 GHz range are the same, on the average. In the case of barred galaxies, however, a definite
dependence is observed between the spectral index and both the IR and × ray luminosities, i.e., the spectral index increases
as both luminosities increase. It is assumed that this is caused by the bar itself, which stimulates star formation in a barred
galaxy.
Translated from Astrofizika, Vol. 41. No. 4, pp. 599–608, October–December, 1998. |
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