Shocked Molecular Gas in the Supernova Remnant HB 21
classification
🌌 astro-ph
keywords
shockedmolecularremnantsupernovaassociatedatomiccorrelationderive
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.