Evolutionary time scales from the AGB to the CSPNe phase

Autores
Miller Bertolami, Marcelo Miguel
Año de publicación
2019
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The transition from the asymptotic giant branch (AGB) to the final white dwarf (WD)stage is arguably the least understood phase in the evolution of single low- and intermediate-mass stars (0.8 ∼ < MZAMS/M ∼ < 8...10). Here we briefly review the progress in the last 50 yearsof the modeling of stars during the post-AGB phase. We show that although the main features,like the extreme mass dependency of post-AGB timescales were already present in the earliestpost-AGB models, the quantitative values of the computed post-AGB timescales changed everytime new physics was included in the modeling of post-AGB stars and their progenitors. Then wediscuss the predictions and uncertainties of the latest available models regarding the evolutionarytimescales of post-AGB stars
Fil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Proceedings of the International Astronomical Union
Viena
Austria
International Astronomical Union
Materia
stars: AGB and post-AGB
stars: evolution
stars: mass loss
planetary nebulae: general
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/210817
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/210817
network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling Evolutionary time scales from the AGB to the CSPNe phaseMiller Bertolami, Marcelo Miguelstars: AGB and post-AGBstars: evolutionstars: mass lossplanetary nebulae: generalhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The transition from the asymptotic giant branch (AGB) to the final white dwarf (WD)stage is arguably the least understood phase in the evolution of single low- and intermediate-mass stars (0.8 ∼ < MZAMS/M ∼ < 8...10). Here we briefly review the progress in the last 50 yearsof the modeling of stars during the post-AGB phase. We show that although the main features,like the extreme mass dependency of post-AGB timescales were already present in the earliestpost-AGB models, the quantitative values of the computed post-AGB timescales changed everytime new physics was included in the modeling of post-AGB stars and their progenitors. Then wediscuss the predictions and uncertainties of the latest available models regarding the evolutionarytimescales of post-AGB starsFil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaProceedings of the International Astronomical UnionVienaAustriaInternational Astronomical UnionCambridge University Press2019info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectSimposioJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/210817Evolutionary time scales from the AGB to the CSPNe phase; Proceedings of the International Astronomical Union; Viena; Austria; 2019; 1-11CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1017/S1743921318007330Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:28:12Zoai:ri.conicet.gov.ar:11336/210817instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:28:13.008CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Evolutionary time scales from the AGB to the CSPNe phase
title Evolutionary time scales from the AGB to the CSPNe phase
spellingShingle Evolutionary time scales from the AGB to the CSPNe phase
Miller Bertolami, Marcelo Miguel
stars: AGB and post-AGB
stars: evolution
stars: mass loss
planetary nebulae: general
title_short Evolutionary time scales from the AGB to the CSPNe phase
title_full Evolutionary time scales from the AGB to the CSPNe phase
title_fullStr Evolutionary time scales from the AGB to the CSPNe phase
title_full_unstemmed Evolutionary time scales from the AGB to the CSPNe phase
title_sort Evolutionary time scales from the AGB to the CSPNe phase
dc.creator.none.fl_str_mv Miller Bertolami, Marcelo Miguel
author Miller Bertolami, Marcelo Miguel
author_facet Miller Bertolami, Marcelo Miguel
author_role author
dc.subject.none.fl_str_mv stars: AGB and post-AGB
stars: evolution
stars: mass loss
planetary nebulae: general
topic stars: AGB and post-AGB
stars: evolution
stars: mass loss
planetary nebulae: general
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The transition from the asymptotic giant branch (AGB) to the final white dwarf (WD)stage is arguably the least understood phase in the evolution of single low- and intermediate-mass stars (0.8 ∼ < MZAMS/M ∼ < 8...10). Here we briefly review the progress in the last 50 yearsof the modeling of stars during the post-AGB phase. We show that although the main features,like the extreme mass dependency of post-AGB timescales were already present in the earliestpost-AGB models, the quantitative values of the computed post-AGB timescales changed everytime new physics was included in the modeling of post-AGB stars and their progenitors. Then wediscuss the predictions and uncertainties of the latest available models regarding the evolutionarytimescales of post-AGB stars
Fil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Proceedings of the International Astronomical Union
Viena
Austria
International Astronomical Union
description The transition from the asymptotic giant branch (AGB) to the final white dwarf (WD)stage is arguably the least understood phase in the evolution of single low- and intermediate-mass stars (0.8 ∼ < MZAMS/M ∼ < 8...10). Here we briefly review the progress in the last 50 yearsof the modeling of stars during the post-AGB phase. We show that although the main features,like the extreme mass dependency of post-AGB timescales were already present in the earliestpost-AGB models, the quantitative values of the computed post-AGB timescales changed everytime new physics was included in the modeling of post-AGB stars and their progenitors. Then wediscuss the predictions and uncertainties of the latest available models regarding the evolutionarytimescales of post-AGB stars
publishDate 2019
dc.date.none.fl_str_mv 2019
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Simposio
Journal
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/210817
Evolutionary time scales from the AGB to the CSPNe phase; Proceedings of the International Astronomical Union; Viena; Austria; 2019; 1-11
CONICET Digital
CONICET
url http://hdl.handle.net/11336/210817
identifier_str_mv Evolutionary time scales from the AGB to the CSPNe phase; Proceedings of the International Astronomical Union; Viena; Austria; 2019; 1-11
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1017/S1743921318007330
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Cambridge University Press
publisher.none.fl_str_mv Cambridge University Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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