Molecular Diagnostics of Supernova Remnant Shocks

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dc.creatorLazendic, J. S.
dc.creatorWardle, M.
dc.creatorGreen, A. J.
dc.creatorWhiteoak, J. B.
dc.creatorBurton, M. G.
dc.date2002-07-18
dc.date.accessioned2026-07-07T02:04:23Z
dc.date.available2026-07-07T02:04:23Z
dc.descriptionWe 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.
dc.description4 pages, 3 figures, appears in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M. Gaensler, 2002, p.399
dc.identifierhttps://arxiv.org/abs/astro-ph/0207406
dc.identifierhttp://arxiv.org/abs/astro-ph/0207406
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4732
dc.subjectAstrophysics
dc.titleMolecular Diagnostics of Supernova Remnant Shocks
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