Modeling the nucleosynthesis of massive stars

dc.contributor.author	Rauscher, T.
dc.date.accessioned	2013-07-02T10:47:01Z
dc.date.available	2013-07-02T10:47:01Z
dc.date.issued	2004-02
dc.identifier.citation	Rauscher , T 2004 , ' Modeling the nucleosynthesis of massive stars ' , New Astronomy Reviews , vol. 48 , no. 1-4 , pp. 3-6 . https://doi.org/10.1016/j.newar.2003.11.002
dc.identifier.issn	1387-6473
dc.identifier.uri	http://hdl.handle.net/2299/11005
dc.description.abstract	This overview discusses issues relevant to modeling nucleosynthesis in type II supernovae and implications of detailed studies of the ejecta. After a brief presentation of the most common approaches to stellar evolution and parameterized explosions, the relevance of a number of nuclei to obtain information on the evolution and explosion mechanisms is discussed. The paper is concluded by an outlook on multi-dimensional simulations. (C) 2003 Elsevier B.V. All rights reserved.	en
dc.format.extent	4
dc.format.extent	92551
dc.language.iso	eng
dc.relation.ispartof	New Astronomy Reviews
dc.subject	NUCLEAR
dc.subject	stars : late stages of evolution
dc.subject	supernovae
dc.subject	EXPLOSION
dc.subject	CORE-COLLAPSE SUPERNOVAE
dc.subject	nucleosynthesis
dc.subject	EVOLUTION
dc.subject	nuclear processes (astrophysics)
dc.title	Modeling the nucleosynthesis of massive stars	en
dc.contributor.institution	Centre for Astrophysics Research
dc.description.status	Peer reviewed
rioxxterms.versionofrecord	10.1016/j.newar.2003.11.002
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true