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Gas Flows in S-E Binary Systems of Galaxies

Published online by Cambridge University Press:  12 April 2016

N. Ya. Sotnikova
N. Ya. Sotnikova*
Affiliation:
Astronomical Observatory, Leningrad State University, Leningrad, USSR

Extract

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Tidal interaction between the galaxies in binary systems leads to important consequences. Some peculiarities in galactic morphology as well as the transfer of matter from one galaxy to another may be due to this factor. In particular, gas flows in intergalactic space may be formed. Such flows enriching one component with gas from the other may play a substantial role in the evolution of mixed (S-E) pairs. One can mention several facts corroborating the possibility of the gas transfer from the spiral to the elliptical galaxy.

Type
IX. Theory of Interaction Stimulated Effects
Information
International Astronomical Union Colloquium , Volume 124: Paired and Interacting Galaxies , 1990 , pp. 717 - 726
Copyright
Copyright © NASA 1990

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