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On Leading Spiral Arms in Close Pairs of Galaxies

Published online by Cambridge University Press:  12 April 2016

A. M. Fridman
A. M. Fridman*
Affiliation:
Astronomical Council of the USSR Academy of Sciences, 48, Pyatnitskaya Stree, 109017 Moscow, USSR

Abstract

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It is explained why one can observe a leading spiral pattern in close pairs of galaxies where the direction of the orbital momentum of the satellite is opposite to the direction of the spin of the spiral galaxy.

Type
VII. Classical Theory of Pairs
Information
International Astronomical Union Colloquium , Volume 124: Paired and Interacting Galaxies , 1990 , pp. 555 - 563
Copyright
Copyright © NASA 1990

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