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dc.date.accessioned 2019-11-22T17:59:10Z
dc.date.available 2019-11-22T17:59:10Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/85972
dc.description.abstract The post-asymptotic giant branch (AGB) phase is arguably one of the least understood phases of the evolution of low- and intermediate- mass stars. The recent post-AGB evolutionary sequences computed by Miller Bertolami (2016) are at least three to ten times faster than those previously published by Vassiliadis & Wood (1994) and Blöcker (1995) which have been used in a large number of studies. This is true for the whole mass and metallicity range. The new models are also ~0.1-0.3 dex brighter than the previous models with similar remnant masses. In this short article we comment on the main reasons behind these differences, and discuss possible implications for other studies of post-AGB stars or planetary nebulae. en
dc.format.extent 179-183 es
dc.language en es
dc.subject planetary nebulae: general es
dc.subject stars: AGB and post-AGB es
dc.title New models for the evolution of central stars of planetary nebulae: faster and brighter en
dc.type Articulo es
sedici.identifier.other doi:10.1017/S1743921317001533 es
sedici.identifier.other eid:2-s2.0-85047006363 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Miller Bertolami, Marcelo Miguel 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 323 (Beijing, China, October 10-14, 2016) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 12, no. S323 es
sedici.rights.sherpa * Color: green * Pre-print del autor: can * Post-print del autor: can * Versión de editor/PDF:cannot * Condiciones: >>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 6 months embargo >>Publisher's version/PDF cannot be used >>Published abstract may be deposited >>Pre-print to record acceptance for publication >>Publisher copyright and source must be acknowledged >>Must link to publisher version or journal website >>Authors may choose to use a Creative Commons Attribution Non-Commercial No Derivatives License >>Publisher last reviewed on 09/10/2014 * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1743-9213/es/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)