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Surprisingly high-pressure shocks in the supernova remnant IC 443
Author(s) -
A. Moorhouse,
P. W. J. L. Brand,
T. R. Geballe,
Michael Burton
Publication year - 1991
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/253.4.662
Subject(s) - physics , supernova remnant , supernova , shock (circulatory) , astrophysics , shock wave , jump , molecular cloud , hydrogen molecule , astronomy , hydrogen , mechanics , stars , medicine , quantum mechanics
The 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.

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