dc.creator |
Bever, J. Van |
|
dc.creator |
Belkus, H. |
|
dc.creator |
Vanbeveren, D. |
|
dc.date.accessioned |
2014-11-14T15:17:01Z |
|
dc.date.available |
2014-11-14T15:17:01Z |
|
dc.date.issued |
2007-04 |
|
dc.identifier.issn |
0004-637X |
|
dc.identifier.issn |
1538-4357 |
|
dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/25907 |
|
dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
Core collapse of dense massive star clusters is unavoidable, and this leads to the formation of massive objects, with masses of up to 1000 M[circled dot] and even larger. When these objects become stars, stellar wind mass loss determines their evolution and final fate, and decides on whether they form black holes (with normal mass or with intermediate mass) or explode as a pair-instability supernova. In this paper we discuss the evolution of very massive stars and present a convenient evolution recipe that can be implemented in a gravitational N-body code to study the dynamics of dense massive clusters. |
en_CA |
dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2014-11-14T15:17:01Z
No. of bitstreams: 1
Bever_J_Van_article_2007.pdf: 319846 bytes, checksum: 15f34e81d7ec8652215e5a394466fcf7 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2014-11-14T15:17:01Z (GMT). No. of bitstreams: 1
Bever_J_Van_article_2007.pdf: 319846 bytes, checksum: 15f34e81d7ec8652215e5a394466fcf7 (MD5)
Previous issue date: 2007-04 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
American Astronomical Society |
en_CA |
dc.relation.uri |
http://dx.doi.org/10.1086/512181 |
|
dc.rights |
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user. |
|
dc.subject.lcsh |
Stars -- Evolution |
|
dc.subject.lcsh |
Supergiant stars |
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dc.subject.lcsh |
Stellar winds |
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dc.title |
The evolution of very massive stars |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Astrophysical Journal 659(2), 1576-1581. (2007) |
en_CA |
Copyright statement:
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.