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XMM Observations of Low Mass GroupsThe contents of this report contains discussion of the two-dimensional XMM-Newton group survey. The analysis of the NGC 2300 and Pavo observations indicated by the azimuthally averaged analysis that the temperature structure is minimal to the NGC2300 system; however, the Pavo system shows signs of a merger in progress. XMM data is used to generate two dimensional maps of the temperature and abundance used to generate maps of pressure and entropy.
Document ID
20050240911
Acquisition Source
Headquarters
Document Type
Preprint (Draft being sent to journal)
Authors
Davis, David S.
(Maryland Univ. Baltimore, MD, United States)
Date Acquired
August 23, 2013
Publication Date
November 9, 2005
Subject Category
Astrophysics
Funding Number(s)
CONTRACT_GRANT: NAG5-12739
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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