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X-ray emission from superbubblesThe results of Rosat observations of superbubbles in the Large Magellanic Cloud provided X-ray spectra for bright objects and data on upper limits of faint objects. The X-ray emission from superbubbles can be used to determine the physical condition of the superbubble interior, place constraints on the ambient interstellar medium, and diagnose the existence of supernova remnant shocks.
Document ID
19970024582
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Chu, You-Hua (Illinois Univ. Urbana, IL United States)
MacLow, Mordecai-Mark (Max-Planck-Inst. fuer Astronomie Heidelberg, Germany)
Date Acquired
August 17, 2013
Publication Date
February 1, 1996
Subject Category
Space Radiation
Accession Number
97N24339
Funding Number(s)
CONTRACT_GRANT: NAGw-4519
CONTRACT_GRANT: NAG5-2679
CONTRACT_GRANT: NAG5-1900
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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