Stellar models including pre-SN/SN phases

Alexander Heger; S. E. Woosley; Norbert Langer

doi:10.1016/S1387-6473(00)00043-9

Stellar models including pre-SN/SN phases

Alexander Heger, S. E. Woosley, Norbert Langer

Research output: Contribution to journal › Review Article › Research › peer-review

6 Citations (Scopus)

Abstract

We present a grid of new models of rotating and non-rotating stars of solar metallicity. Their evolution was followed form the pre-main sequence stage up to core collapse using a 199 isotope network. The evolution and nucleosynthesis was continued through the supernova stage using a 'piston' model [Woosley, S.E, Weaver, T.A., 1995, ApJS, 101, 181] to simulate the explosion. Final isotopic yields are given for 15 and 25 M_ȯ stars with different assumptions regarding the mixing efficiency of semiconvection and for rotating and non-rotating stellar models.

Original language	English
Pages (from-to)	297-302
Number of pages	6
Journal	New Astronomy Reviews
Volume	44
Issue number	4-6
DOIs	https://doi.org/10.1016/S1387-6473(00)00043-9
Publication status	Published - 1 Jan 2000
Externally published	Yes

Keywords

Nucleosynthesis
Rotation
Stellar evolution
Supernovae

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10.1016/S1387-6473(00)00043-9

Cite this

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title = "Stellar models including pre-SN/SN phases",

abstract = "We present a grid of new models of rotating and non-rotating stars of solar metallicity. Their evolution was followed form the pre-main sequence stage up to core collapse using a 199 isotope network. The evolution and nucleosynthesis was continued through the supernova stage using a 'piston' model [Woosley, S.E, Weaver, T.A., 1995, ApJS, 101, 181] to simulate the explosion. Final isotopic yields are given for 15 and 25 Mȯ stars with different assumptions regarding the mixing efficiency of semiconvection and for rotating and non-rotating stellar models.",

keywords = "Nucleosynthesis, Rotation, Stellar evolution, Supernovae",

author = "Alexander Heger and Woosley, \{S. E.\} and Norbert Langer",

year = "2000",

month = jan,

day = "1",

doi = "10.1016/S1387-6473(00)00043-9",

language = "English",

volume = "44",

pages = "297--302",

journal = "New Astronomy Reviews",

issn = "1387-6473",

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number = "4-6",

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TY - JOUR

T1 - Stellar models including pre-SN/SN phases

AU - Heger, Alexander

AU - Woosley, S. E.

AU - Langer, Norbert

PY - 2000/1/1

Y1 - 2000/1/1

N2 - We present a grid of new models of rotating and non-rotating stars of solar metallicity. Their evolution was followed form the pre-main sequence stage up to core collapse using a 199 isotope network. The evolution and nucleosynthesis was continued through the supernova stage using a 'piston' model [Woosley, S.E, Weaver, T.A., 1995, ApJS, 101, 181] to simulate the explosion. Final isotopic yields are given for 15 and 25 Mȯ stars with different assumptions regarding the mixing efficiency of semiconvection and for rotating and non-rotating stellar models.

AB - We present a grid of new models of rotating and non-rotating stars of solar metallicity. Their evolution was followed form the pre-main sequence stage up to core collapse using a 199 isotope network. The evolution and nucleosynthesis was continued through the supernova stage using a 'piston' model [Woosley, S.E, Weaver, T.A., 1995, ApJS, 101, 181] to simulate the explosion. Final isotopic yields are given for 15 and 25 Mȯ stars with different assumptions regarding the mixing efficiency of semiconvection and for rotating and non-rotating stellar models.

KW - Nucleosynthesis

KW - Rotation

KW - Stellar evolution

KW - Supernovae

UR - https://www.scopus.com/pages/publications/0042139646

U2 - 10.1016/S1387-6473(00)00043-9

DO - 10.1016/S1387-6473(00)00043-9

M3 - Review Article

AN - SCOPUS:0042139646

SN - 1387-6473

VL - 44

SP - 297

EP - 302

JO - New Astronomy Reviews

JF - New Astronomy Reviews

IS - 4-6

ER -

Stellar models including pre-SN/SN phases

Abstract

Keywords

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