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dc.contributor.author
Benvenuto, Omar Gustavo
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Panei, Jorge Alejandro
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Nomoto, Ken’ichi
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Kitamura, Hikaru
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Hachisu, Izumi
dc.date.available
2017-02-07T13:41:50Z
dc.date.issued
2015-08
dc.identifier.citation
Benvenuto, Omar Gustavo; Panei, Jorge Alejandro; Nomoto, Ken’ichi ; Kitamura, Hikaru; Hachisu, Izumi; Final evolution and delayed explosions of spinning white dwarfs in single degenerate models for type Ia supernovae; Iop Publishing; Astrophysical Journal; 809; L6; 8-2015; 6-10
dc.identifier.issn
0004-637X
dc.identifier.uri
http://hdl.handle.net/11336/12613
dc.description.abstract
We study the occurrence of delayed SNe Ia in the single degenerate (SD) scenario. We assume that a massive carbon-oxygen (CO) white dwarf (WD) accretes matter coming from a companion star, making it to spin at the critical rate. We assume uniform rotation due to magnetic field coupling.NR The carbon ignition mass for non-rotating WDs is M ig ≈ 1.38 M ⊙ ; while for the case of uniformly R rotating WDs it is a few percent larger (M ig ≈ 1.43 M ⊙ ). When accretion rate decreases, the WD begins to lose angular momentum, shrinks, and spins up; however, it does not overflow its critical rotation rate, avoiding mass shedding. Thus, angular momentum losses can lead the CO WD interior to compression and carbon ignition, which would induce an SN Ia. The delay, largely due to the angular momentum losses timescale, may be large enough to allow the companion star to evolve to a He WD, becoming undetectable at the moment of explosion. This scenario supports the occurrence of delayed SNe Ia if the final CO WD mass is 1.38 Msun < M < 1.43 Msun . We also find that if the delay is longer than ∼ 3 Gyr, the WD would become too cold to explode, rather undergoing collapse.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Iop Publishing
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Close Binaries
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Supernovae
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Nuclear Reactions
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Nucleosynthesis
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Abundances
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Star Rotation
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White Dwarfs
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Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Final evolution and delayed explosions of spinning white dwarfs in single degenerate models for type Ia supernovae
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-01-11T13:26:30Z
dc.journal.volume
809
dc.journal.number
L6
dc.journal.pagination
6-10
dc.journal.pais
Estados Unidos
dc.description.fil
Fil: Benvenuto, Omar Gustavo. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina
dc.description.fil
Fil: Panei, Jorge Alejandro. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
dc.description.fil
Fil: Nomoto, Ken’ichi . University of Tokyo. Kavli Institute for the Physics and Mathematics of the Universe; Japón
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Fil: Kitamura, Hikaru. Kyoto University. Department of Physics; Japón
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Fil: Hachisu, Izumi. The University of Tokyo; Japón
dc.journal.title
Astrophysical Journal
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/809/1/L6/meta
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/2041-8205/809/1/L6
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