Shocked Interstellar clouds and dust grain destruction in the LMC Supernova Remnant N132D
Shocked Interstellar clouds and dust grain destruction in the LMC Supernova Remnant N132D
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
From integral field data we extract the optical spectra of 20 shocked clouds in the supernova remnant N132D in the Large Magellanic Cloud (LMC). Using self-consistent shock modelling, we derive the shock velocity, pre-shock cloud density and shock ram pressure in these clouds. We show that the [Fe X] and [Fe XIV] emission arises in faster, partiall...
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Full title
Shocked Interstellar clouds and dust grain destruction in the LMC Supernova Remnant N132D
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TN_cdi_proquest_journals_2073451539
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073451539
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1806.04276
