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Cosmic supernova rate history and Type Ia supernova progenitors

dc.contributor.authorNomoto, K
dc.contributor.authorTsujimoto, T
dc.contributor.authorKobayashi, Chiaki
dc.contributor.editorVangioni-Flam, E
dc.contributor.editorFerlet, R
dc.contributor.editorLemoine, M
dc.date.accessioned2011-12-20T12:01:09Z
dc.date.available2011-12-20T12:01:09Z
dc.date.issued2001
dc.identifier.citationNomoto , K , Tsujimoto , T & Kobayashi , C 2001 , Cosmic supernova rate history and Type Ia supernova progenitors . in E Vangioni-Flam , R Ferlet & M Lemoine (eds) , Cosmic Evolution . World Scientific Publishing , SINGAPORE , pp. 313-316 , Symposium on Cosmic Evolution , PARIS , 13/11/00 .
dc.identifier.citationconference
dc.identifier.isbn981-02-4786-9
dc.identifier.isbn9789810247867
dc.identifier.otherPURE: 496846
dc.identifier.otherPURE UUID: a851e86e-2e76-466a-a25e-d180c9f75f2d
dc.identifier.otherWOS: 000173048600073
dc.identifier.otherORCID: /0000-0002-4343-0487/work/62750450
dc.identifier.urihttp://hdl.handle.net/2299/7403
dc.description.abstractAdopting a single degenerate scenario for Type Ia supernova progenitors with the metallicity effect, we make a prediction of the cosmic supernova rate history as a composite of the supernova rates in spiral and elliptical galaxies, and compare with the recent observational data up to z similar to 0.55.en
dc.format.extent4
dc.language.isoeng
dc.publisherWorld Scientific Publishing
dc.relation.ispartofCosmic Evolution
dc.subjectEVOLUTION
dc.subjectCHANNEL
dc.titleCosmic supernova rate history and Type Ia supernova progenitorsen
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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