Three-dimensional hydrodynamics simulations of shell burning in Si/O-rich layer of pre-collapse mass...
Three-dimensional hydrodynamics simulations of shell burning in Si/O-rich layer of pre-collapse massive stars
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Les Ulis: EDP Sciences
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Language
English
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Les Ulis: EDP Sciences
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We perform three-dimensional (3D)hydrodynamics simulations of shell burning in the silicon-and oxygen-rich layers in pre-collapse massive stars.Weadoptanon-rotating27
M
⊙
starhaving anextended O/Si/Ne layer and afast-rotating 38
M
⊙
star having a Si/Olayer, that has experienced chemically homogeneousevolution. Both pre-collapse st...
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Three-dimensional hydrodynamics simulations of shell burning in Si/O-rich layer of pre-collapse massive stars
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TN_cdi_doaj_primary_oai_doaj_org_article_db16031ef94442d7abc9ee291562e53f
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_db16031ef94442d7abc9ee291562e53f
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ISSN
2100-014X,2101-6275
E-ISSN
2100-014X
DOI
10.1051/epjconf/202226011038