Shocked Molecular Gas in the Supernova Remnant HB 21
Preprint
- 15 December 2000
Abstract
We report the discovery of the shocked molecular gas in the supernova remnant HB 21. We derive the physical parameters of the shocked gas from CO J=1-0 and J=2-1 line observations. We discuss the correlation of the shocked molecular gas with the previously detected, shocked atomic gas and the associated infrared emission.Keywords
All Related Versions
- Version 1, 2000-12-15, ArXiv
- Published version: The Astrophysical Journal, 552 (1), 175.
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