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dc.date.accessioned | 2021-10-26T18:18:37Z | |
dc.date.available | 2021-10-26T18:18:37Z | |
dc.date.issued | 2015-08 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/127319 | |
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. The carbon ignition mass for non-rotating WDs is MigNR ≈ 1.38 M⊙; while for the case of uniformly rotating WDs it is a few percent larger (MigR ≈ 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 M⊙ < M < 1.43 M⊙. We also find that if the delay is longer than ~3 Gyr, the WD would become too cold to explode, rather undergoing collapse. | en |
dc.language | en | es |
dc.subject | binaries: close | es |
dc.subject | nuclear reactions, nucleosynthesis, abundances | es |
dc.subject | stars: rotation | es |
dc.subject | supernovae: general | es |
dc.subject | white dwarfs | es |
dc.title | Final Evolution and Delayed Explosions of Spinning White Dwarfs in Single Degenerate Models for Type Ia Supernovae | en |
dc.type | Articulo | es |
sedici.identifier.other | arXiv:1508.01921v1 | es |
sedici.identifier.other | doi:10.1088/2041-8205/809/1/l6 | es |
sedici.identifier.issn | 2041-8213 | es |
sedici.identifier.issn | 2041-8205 | es |
sedici.creator.person | Benvenuto, Omar Gustavo | es |
sedici.creator.person | Panei, Jorge Alejandro | es |
sedici.creator.person | Nomoto, Ken'ichi | es |
sedici.creator.person | Kitamura, Hikaru | es |
sedici.creator.person | Hachisu, Izumi | es |
sedici.subject.materias | Astronomía | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Facultad de Ciencias Astronómicas y Geofísicas | es |
mods.originInfo.place | Instituto de Astrofísica de La Plata | es |
sedici.subtype | Articulo | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.description.peerReview | peer-review | es |
sedici.workflowEdited | true | es |
sedici.relation.journalTitle | The Astrophysical Journal Letters | es |
sedici.relation.journalVolumeAndIssue | vol. 809, no. 1 | es |