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The X-ray superbubble in CygnusIt is shown that Cyg X-6 and Cyg X-7 are part of a large X-ray ring, 13 degrees in diameter. At a distance of 2 kpc, this X-ray source lies behind the Great Rift of Cygnus, and as such has radiation from its central region absorbed. The diameter of the emitting region is 450 pc. The X-ray source is associated with a ring of elongated H-alpha filaments which enclose the Cygnus X radio source. At the center of this region lies the highly luminous Cygnus OB2 association.
Document ID
19800060821
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cash, W.
(Colorado, University Boulder, Colo., United States)
Charles, P.
(Colorado Univ. Boulder, CO, United States)
Bowyer, S.
(Colorado Univ. Boulder, CO, United States)
Walter, F.
(California, University Berkeley, Calif., United States)
Garmire, G.
(California Institute of Technology Pasadena, Calif., United States)
Riegler, G.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 10, 2013
Publication Date
June 1, 1980
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
80A44991
Funding Number(s)
CONTRACT_GRANT: CIT-44-466866
CONTRACT_GRANT: NSG-5303
Distribution Limits
Public
Copyright
Other

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