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The X-ray emission of E and S0 Galaxies

Published online by Cambridge University Press:  25 May 2016

G. Fabbiano
G. Fabbiano*
Affiliation:
Harvard-Smithsonian CfA, 60 Garden St., Cambridge MA 02138, USA

Extract

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It is well known by now that E and S0 galaxies are associated with hot, X-ray emitting gaseous halos, subject to central cooling flows, but otherwise homogeneous, which can be used to trace the galaxy potential and thus measure the total gravitational mass. Recent ASCA observations suggest that these halos have a surprisingly low metal abundance.

Type
The Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 123 - 130
Copyright
Copyright © Kluwer 1996 

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