On Leading Spiral Arms in Close Pairs of Galaxies-Reference-Cited by-同舟云学术

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On Leading Spiral Arms in Close Pairs of Galaxies

Published:1990 Issue: Volume:124 Page:555-563
ISSN:0252-9211
Container-title:International Astronomical Union Colloquium
language:en
Short-container-title:International Astronomical Union Colloquium

Author:

Fridman A. M.

Abstract

AbstractIt 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.

Publisher

Cambridge University Press (CUP)

Reference15 articles.

1. Werner D. A. 1956, Astron. Tsirk., 1466, 5.

2. Tilt Criteria and Direction of Rotation of Spiral Galaxies.

3. On the Direction of Rotation in Spiral Nebulae.

4. On the Hydrodynamical Conception of the Spiral Structure in Galaxies with a Velocity “Kink” on the Rotation Curve (Theory, Laboratory Experiments, Numerical Simulation, Observations)

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