Molecular Diagnostics of Supernova Remnant Shocks

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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.
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

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Astrophysics

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https://dspace.dare.co.zw/handle/123456789/5591

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arXiv

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