Molecular Diagnostics of Supernova Remnant Shocks
Abstract
We have undertaken a study of radio and infrared molecular-line emission towards several SNRs in order to investigate molecular signatures of SNR shocks, and to test models for OH maser production in SNRs. Here we present results on G349.7+0.2.
- Publication:
-
Neutron Stars in Supernova Remnants
- Pub Date:
- 2002
- DOI:
- arXiv:
- arXiv:astro-ph/0207406
- Bibcode:
- 2002ASPC..271..399L
- Keywords:
-
- Astrophysics
- E-Print:
- 4 pages, 3 figures, appears in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M. Gaensler, 2002, p.399