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The Large Scale X-Ray Emission from M87We describe asymmetrical features in a long exposure X-ray map of M87 made with the ROSAT High Resolution Imager (HRI). A bright triangular region is marked by a linear 'spur' along one edge. The structure of this spur suggests an interpretation of a tangential view of a shock front 18 kpc long. None of the brighter features are spatially coincident with radio or optical structures so we concur with earlier investigators that most of the emission arises from thermal processes.
Document ID
20000057334
Acquisition Source
Goddard Space Flight Center
Document Type
Other
Authors
Harris, D. E.
(Smithsonian Astrophysical Observatory Cambridge, MA United States)
Biretta, J. A.
(Space Telescope Science Inst. Baltimore, MD United States)
Junor, W.
(New Mexico Univ. Albuquerque, NM United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 1998
Subject Category
Space Radiation
Funding Number(s)
CONTRACT_GRANT: NAG5-2957
CONTRACT_GRANT: NAG5-2960
CONTRACT_GRANT: NAS5-30934
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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