Show simple item record

Nucleosynthesis in supernovae

dc.contributor.authorThielemann, Friedrich-Karl
dc.contributor.authorArgast, D.
dc.contributor.authorBrachwitz, F.
dc.contributor.authorMartinez-Pinedo, Gabriel
dc.contributor.authorRauscher, T.
dc.contributor.authorLiebendoerfer, M.
dc.contributor.authorMezzacappa, A.
dc.contributor.authorHoflich, P.
dc.contributor.authorIwamoto, K.
dc.contributor.authorNomoto, K.
dc.contributor.editorFusco Femiano, R.
dc.contributor.editorMatteucci, F.
dc.date.accessioned2014-11-27T09:14:31Z
dc.date.available2014-11-27T09:14:31Z
dc.date.issued2002
dc.identifier.citationThielemann , F-K , Argast , D , Brachwitz , F , Martinez-Pinedo , G , Rauscher , T , Liebendoerfer , M , Mezzacappa , A , Hoflich , P , Iwamoto , K & Nomoto , K 2002 , Nucleosynthesis in supernovae . in R Fusco Femiano & F Matteucci (eds) , Chemical Enrichment of Intracluster and Intergalactic Medium . ASP Conf Series , vol. 253 , Astronomical Society of the Pacific , San Francisco , pp. 205-218 , Meeting on Chemical Enrichment of Intracluster and Intergalactic Medium , VULCANO , Italy , 14/05/01 . < http://www.aspbooks.org/publications/253/205.pdf >
dc.identifier.citationconference
dc.identifier.isbn1-58381-093-5
dc.identifier.isbn978-1-58381-589-2
dc.identifier.otherPURE: 1633385
dc.identifier.otherPURE UUID: 51d9030b-08c1-4927-bcd4-d0a51fe96166
dc.identifier.otherWOS: 000176731700023
dc.identifier.urihttp://hdl.handle.net/2299/14824
dc.description.abstractThe evolution of gas abundances in galaxies and the enrichment of heavy elements as a function of space and time reflects the history of star formation and the lifetimes of the diverse contributing stellar objects. Supernovae of type la and type II/Ib/Ic are the main contributors to nucleosynthesis in galaxies. Despite many efforts, a full and self-consistent understanding of supernova explosion mechanisms is not existing, yet. However, they leave fingerprints, seen either in spectra, lightcurves, radioactivities/decay gamma-rays or in galactic evolution. Here we want to address the relation of model uncertainties to the composition of ejecta and test them with constraints from abundance observations.en
dc.format.extent14
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofChemical Enrichment of Intracluster and Intergalactic Medium
dc.relation.ispartofseriesASP Conf Series
dc.subjectWEAK INTERACTION RATES
dc.subjectR-PROCESS NUCLEOSYNTHESIS
dc.subjectIA SUPERNOVAE
dc.subjectCARBON DEFLAGRATION SUPERNOVAE
dc.subjectII SUPERNOVAE
dc.subjectMETAL-POOR STARS
dc.subjectROTATING MASSIVE STARS
dc.subjectNEUTRINO-DRIVEN WINDS
dc.subjectCORE-COLLAPSE SUPERNOVAE
dc.subjectCIRCLE-DOT STAR
dc.titleNucleosynthesis in supernovaeen
dc.contributor.institutionCentre for Astrophysics Research
dc.identifier.urlhttp://www.aspbooks.org/publications/253/205.pdf
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record