H2 in molecular shocks: observations from 2 to 12 microns

Details H2 in molecular shocks: observations from 2 to 12 microns H2 in molecular shocks: observations from 2 to 12 microns

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.233...67r&link_type=abstract

Astrophysics and Space Science, Volume 233, Issue 1-2, pp. 67-70

Astronomy and Astrophysics

Astrophysics

Interstellar Molecules, Supernova Remnants, Infrared Spectroscopy

Scientific paper

We present spectroscopy of the molecular shock in the supernova remnant IC 443. The H2 level populations in IC 443 are nearly identical to Orion Peak 1 (Brand et al. 1988; Parmar et al. 1994) and are consistent with a partially dissociative J-shock. The similarity with Orion suggests the shock processes which dominate the emission in both regions are essentially identical.

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