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A Dynamical Proximity Analysis of Interacting Galaxy Pairs

Published online by Cambridge University Press:  12 April 2016

Tapan K. Chatterjee*
Affiliation:
Facultad de Ciencias, Fisico-Matematicas, Universidad A. Puebla, (A.P. 1152), Puebla, Mexico

Abstract

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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
Copyright
Copyright © NASA 1990

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