Infrared spectroscopy of supernova remnants

Details Infrared spectroscopy of supernova remnants Infrared spectroscopy of supernova remnants

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...214..307o&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 214, no. 1-2, April 1989, p. 307-320.

Astronomy and Astrophysics

Astrophysics

94

Crab Nebula, Hydrogen Recombinations, Infrared Spectroscopy, Magellanic Clouds, Supernova Remnants, Astronomical Maps, H Ii Regions, Spatial Distribution

Scientific paper

The results of a systematic study of IR spectra of supernova remnants are presented. Prominent molecular hydrogen lines were detected over a large region extending beyond the optical emission in RCW 103 suggesting an interaction between this remnant and a molecular cloud. The forbidden Fe II transition at 1.6435 microns was found to be a prominent feature in all of the remnants observed. The observed fluxes of hydrogen lines in the IR cannot be reconciled with the measurements of H-alpha and H-beta.

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