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X-ray image of the Cygnus LoopAn X-ray picture of the Cygnus Loop, recorded with an imaging X-ray telescope, is presented. The results are highly suggestive of a limb-brightened shell of hot gas which results from the expansion of a blast wave into the interstellar medium. Spatial structure is clearly evident on scale sizes down to about 1/4 deg, a likely indication of the inhomogeneities in the interstellar medium. No evidence is found for any discrete X-ray-emitting remnant of the original supernova explosion.
Document ID
19790036167
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Rappaport, S.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Petre, R.
(MIT Cambridge, Mass., United States)
Kayat, M. A.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Evans, K. D.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Smith, G. C.
(Leicester, University Leicester, United Kingdom)
Levine, A.
(Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1979
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
79A20180
Funding Number(s)
CONTRACT_GRANT: SRC-SG/B/00440
CONTRACT_GRANT: NGR-22-009-730
Distribution Limits
Public
Copyright
Other

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