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Surprisingly high-pressure shocks in the supernova remnant IC 443The intensities of several lines of molecular hydrogen have been measured from two regions of the supernova-remnant/molecular-cloud shock in IC 443. The lines measured have upper-state energies ranging from 7000 K to 23,000 K. Their relative intensities differ in the two regions, but are consistent with those predicted from the post-shock regions of simple jump-type shocks of different pressure. The pressures so derived are far higher than the pressure in the supernova remnant itself, and a possible reason for this discrepancy is discussed.
Document ID
19920037389
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Moorhouse, A.
(Royal Observatory Edinburgh, United Kingdom)
Brand, P. W. J. L.
(Royal Observatory Edinburgh, United Kingdom)
Geballe, T. R.
(Joint Astronomy Center Hilo, HI, United States)
Burton, M. G.
(NASA Ames Research Center Moffett Field; California, University, Irvine, United States)
Date Acquired
August 15, 2013
Publication Date
December 15, 1991
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 253
ISSN: 0035-8711
Subject Category
Astrophysics
Accession Number
92A20013
Distribution Limits
Public
Copyright
Other

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