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dc.contributor.authorKobayashi, C.
dc.contributor.authorNomoto, K. I.
dc.contributor.editorHillebrandt, W.
dc.contributor.editorLeibundgut, B.
dc.date.accessioned2015-01-12T10:02:38Z
dc.date.available2015-01-12T10:02:38Z
dc.date.issued2003
dc.identifier.citationKobayashi , C & Nomoto , K I 2003 , Type Ia supernova progenitors, lifetime, and cosmic supernova rate . in W Hillebrandt & B Leibundgut (eds) , From Twilight to Highlight : the Physics of Supernovae . Springer Nature , Berlin , pp. 379-383 , Workshop on From Twilight to Highlights - The Physics of Supernovae , Garching , Germany , 29/07/02 .
dc.identifier.citationconference
dc.identifier.isbn3-540-00483-1
dc.identifier.isbn978-3540004837
dc.identifier.otherPURE: 811313
dc.identifier.otherPURE UUID: 7ba73724-51c5-436b-9c0b-a16daf5d8d25
dc.identifier.otherWOS: 000182974600051
dc.identifier.otherORCID: /0000-0002-4343-0487/work/62750494
dc.identifier.urihttp://hdl.handle.net/2299/15153
dc.description.abstractWe make a comparison of the lifetime distribution derived from several models of Type Ia Supernovae (SNe Ia) and evaluate the SN Ia models from the observational constraints. Our SN Ia model, which is based on the single degenerate scenario and includes the metallicity effect, gives better reproduction of the [O/Fe]-(Fe/H) relation in the solar neighborhood if compared to, e.g., Matteucci & Recchi (2001). We also provide predictions of the cosmic supernova rate history.en
dc.format.extent5
dc.language.isoeng
dc.publisherSpringer Nature
dc.relation.ispartofFrom Twilight to Highlight
dc.subjectEVOLUTION
dc.subjectGALAXIES
dc.titleType Ia supernova progenitors, lifetime, and cosmic supernova rateen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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