Roman CCS White Paper: Characterizing Superluminous Supernovae with Roman
Roman CCS White Paper: Characterizing Superluminous Supernovae with Roman
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Author / Creator
Gomez, Sebastian , Alexander, Kate , Berger, Edo , Blanchard, Peter K , Broekgaarden, Floor , Eftekhari, Tarraneh , Fox, Ori , Gill, Kiranjyot , Hiramatsu, Daichi , Joshi, Bhavin , Mitchell, Karmen , Moriya, Takashi , Nicholl, Matt , Quimby, Robert , Regos, Eniko , Rest, Armin , Rose, Benjamin , Shahbandeh, Melissa and Villar, V Ashley
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
Type-I Superluminous Supernovae (SLSNe) are an exotic class of core-collapse SN (CCSN) that can be up to 100 times brighter and more slowly-evolving than normal CCSNe. SLSNe represent the end-stages of the most massive stripped stars, and are thought to be powered by the spin-down energy of a millisecond magnetar. Studying them and measuring their...
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Roman CCS White Paper: Characterizing Superluminous Supernovae with Roman
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Record Identifier
TN_cdi_proquest_journals_2832637830
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2832637830
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E-ISSN
2331-8422
