Fe K and ejecta emission in SNR G15.9+0.2 with XMM-Newton
Fe K and ejecta emission in SNR G15.9+0.2 with XMM-Newton
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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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Aims: We present a study of the Galactic supernova remnant SNR G15.9+0.2 with archival XMM-Newton observations. Methods: EPIC data are used to investigate the morphological and spectral properties of the remnant, searching in particular for supernova ejecta and Fe K line emission. By comparing the SNR's X-ray absorption column density with the atom...
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Fe K and ejecta emission in SNR G15.9+0.2 with XMM-Newton
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TN_cdi_proquest_journals_2074799489
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2074799489
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1611.02191
