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Interstellar Matter in Elliptical Galaxies

Published online by Cambridge University Press:  04 August 2017

G. R. Knapp
G. R. Knapp*
Affiliation:
Princeton University Observatory, Princeton, NJ08544, U.S.A.

Extract

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This contribution concentrates on the properties of the large gas structures in elliptical galaxies, those seen in dust and HI. The distribution and kinematics of ionized gas, which is generally confined to a small region in the center of the galaxy, are discussed at this conference by Illingworth and by Ulrich.

Type
V. Spheroidal Systems
Information
Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 297 - 304
Copyright
Copyright © Reidel 1983 

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