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Excitation and Disruption of a Giant Molecular Cloud by the Sepurnova Remnant 3C 391The ambient molecular gas at the distance of the remnant comprises a giant molecular cloud whose edge is closely parallel to a ridge of bright non-thermal radio continuum, which evidently delineates the blast-wave into the cloud.
Document ID
20060041301
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Reach, W. T.
Rho, J.
Date Acquired
August 23, 2013
Publication Date
May 1, 1998
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
giant molecular cloud supernova remnants ISM radio 3C 391 structure radio lines

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