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Chandra Observations of Clusters of Galaxies

Published online by Cambridge University Press:  30 March 2016

W. Forman ,
H. Donnelly ,
M. Markevitch ,
R. Kraft ,
S. Murray ,
A. Vikhlinin ,
E. Churazov ,
L. David  and
C. Jones
W. Forman
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138
H. Donnelly
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138
M. Markevitch
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138
R. Kraft
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138
S. Murray
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138
A. Vikhlinin
Affiliation:
Institute for Space Research, Profsouznaya 84/32, 117810 Moscow, Russia
E. Churazov
Affiliation:
Institute for Space Research, Profsouznaya 84/32, 117810 Moscow, Russia MPI fur Astrophysik, Karl-Schwartzschild Strasse 1, 85740 Garching, Germany
L. David
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138
C. Jones
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138

Abstract

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We discuss two themes from Chandra cluster observations. First, we describe the interaction of buoyant, radio emitting plasma bubbles with the hot intracluster gas. Second we summarize the Chandra observations of “cold” fronts (sharp discontinuities in gas density and temperature) separating cool, denser gas clouds from the hotter intracluster medium.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 12: Highlights of Astronomy. As presented at the XXIVth General Assembly of the IAU, 2000 , 2002 , pp. 504 - 506
Copyright
Copyright © Astronomical Society of Pacific 2002

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