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dc.date.accessioned | 2019-12-12T18:42:42Z | |
dc.date.available | 2019-12-12T18:42:42Z | |
dc.date.issued | 2016 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/87335 | |
dc.description.abstract | A very active area of research in the field of core-collapse supernovae (SNe) is the study of their progenitors and the links with different subtypes. Direct identification using pre- and post-SN images is a powerful method but it can only be applied to the most nearby events. An alternative method is the hydrodynamical modeling of SN light curves and expansion velocities, which can serve to characterize the progenitor (e.g. mass and radius) and the explosion itself (e.g. explosion energy and radioactive yields). This latter methodology is particularly powerful when combined with stellar evolution calculations. We review our current understanding of the properties of normal core-collapse SNe based chiefly on these two methods. | en |
dc.format.extent | 25-31 | es |
dc.language | en | es |
dc.subject | binaries: general | es |
dc.subject | supernovae: general | es |
dc.title | Core-collape supernova progenitors: Light-curve and stellar-evolution models | en |
dc.type | Articulo | es |
sedici.identifier.other | doi:10.1017/S1743921317003271 | es |
sedici.identifier.other | eid:2-s2.0-85047488543 | es |
sedici.identifier.issn | 1743-9213 | es |
sedici.creator.person | Bersten, Melina Cecilia | es |
sedici.subject.materias | Ciencias Astronómicas | es |
sedici.description.fulltext | true | 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.relation.event | IAU Symposium 329 (Auckland, New Zealand, 2016) | es |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Proceedings of the International Astronomical Union | es |
sedici.relation.journalVolumeAndIssue | vol. 12, no. S329 | es |
sedici.rights.sherpa | * Color: green
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>>Author's Pre-print on author's personal website, departmental website, social media websites, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv
>>Author's post-print on author's personal website on acceptance of publication
>>Author's post-print on departmental website, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv, after a |