Constraining the Hottest Temperature Component of A754 with RXTE

Details Constraining the Hottest Temperature Component of A754 with RXTE Constraining the Hottest Temperature Component of A754 with RXTE

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.4201v&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #42.01; Bulletin of the American Astronomical Society, Vol. 30, p.872

Astronomy and Astrophysics

Astronomy

Scientific paper

A754 was observed with RXTE PCA and HEXTE (2-250 keV combined bandpass) in order to 1) constrain the hottest temperature component of its intracluster medium, and 2) find evidence for non-thermal emission from the cluster. From previous observations, there is ample evidence that A754 is the result of a merger event. A super hot component of the gas is expected to exist as a result of hydrodynamical processes such as shocks. We present our results and discuss their implications.

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