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X-ray structure of the Cygnus loopAn X-ray surface brightness map of the Cygnus Loop in the energy range 0.15-0.85 keV is presented. The X-ray distribution is compared with the optical and radio pictures of the Loop. The location of the center of the supernova shell as derived from the X-ray data is in excellent agreement with the apparent optical and radio centers. We obtain a mean diameter for the X-ray shell of 2.75 (+ or - 0.2) deg. The X-ray spectral data yield a characteristic thermal temperature averaged over the Loop of 2.9 million (+ or - 1.5 million) K. We have calculated anew X-ray parameters for adiabatic blast waves using X-ray production spectra which include line radiation. These parameters are compared with the results of the present experiment. An age of 18,000 years, initial blast energy equal to 3 times 10 to the 50-th power ergs, and ambient interstellar density of 0.25 per cu cm are found.
Document ID
19750032693
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Rappaport, S.
Doxsey, R.
Solinger, A.
(MIT Cambridge, Mass., United States)
Borken, R.
(Wisconsin, University Madison, Wis., United States)
Date Acquired
August 8, 2013
Publication Date
December 1, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 194
Subject Category
Astrophysics
Accession Number
75A16765
Funding Number(s)
CONTRACT_GRANT: NGL-22-009-015
CONTRACT_GRANT: NSF GP-30860X
CONTRACT_GRANT: NSR-22-009-654
Distribution Limits
Public
Copyright
Other

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