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dc.date.accessioned | 2019-12-06T18:18:00Z | |
dc.date.available | 2019-12-06T18:18:00Z | |
dc.date.issued | 2016 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/87018 | |
dc.description.abstract | SAO 244567 is an unusually fast evolving star. Within twenty years only, it had turned from a B-type supergiant into the central star of the Stingray Nebula. Space- and ground-based observations obtained over the last decades have revealed that its spectrum changes noticeably over just a few years, showing stellar evolution in real time. The low mass of SAO 244567 is, however, in strong contradiction with canonical post-asymptotic giant branch evolution. Thus, its fast evolution has been a mystery for decades. We present preliminary results of the non-LTE spectral analyis of the recently obtained HST/COS observations, which finally allow us to shed light on the evolutionary history of this extraordinary object. | en |
dc.language | en | es |
dc.subject | Central star | es |
dc.subject | Stingray Nebula | es |
dc.title | The rapid evolution of the central star of the Stingray Nebula - latest news from the HST | en |
dc.type | Articulo | es |
sedici.identifier.other | doi:10.1088/1742-6596/728/3/032006 | es |
sedici.identifier.other | eid:2-s2.0-84989313956 | es |
sedici.identifier.issn | 1742-6588 | es |
sedici.creator.person | Reindl, Nicole | es |
sedici.creator.person | Rauch, Thomas | es |
sedici.creator.person | Miller Bertolami, Marcelo Miguel | es |
sedici.creator.person | Werner, Klaus | es |
sedici.subject.materias | Ciencias Astronómicas | 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 3.0 Unported (CC BY 3.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by/3.0/ | |
sedici.relation.event | 11th Pacific Rim Conference on Stellar Astrophysics: Physics and Chemistry of the Late Stages of Stellar Evolution (Hong Kong, PR China, 14-17 December, 2015) | es |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Journal of Physics: Conference Series | es |
sedici.relation.journalVolumeAndIssue | vol. 728, no. 3 | es |
sedici.rights.sherpa | * Color: green * Pre-print del autor: can * Post-print del autor: can * Versión de editor/PDF:can * Condiciones: >>On open access repositories and websites >>Creative Commons Attribution License 3.0 >>Published source must be acknowledged >>Publisher's version/PDF may be used >>Publisher last contacted on 17/02/2014 >>All titles are open access journals * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1742-6588/es/ |