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A Dynamical Proximity Analysis of Interacting Galaxy Pairs
Published online by Cambridge University Press: 12 April 2016
Abstract
Using the impulsive approximation to study the velocity changes of stars during disk-sphere collisions and a method due to Bottlinger to study the post collision orbits of stars, the formation of various types of interacting galaxies is studied as a function of the distance of closest approach between the two galaxies.
- Type
- VII. Classical Theory of Pairs
- Information
- International Astronomical Union Colloquium , Volume 124: Paired and Interacting Galaxies , 1990 , pp. 569 - 575
- Copyright
- Copyright © NASA 1990