Exploring massive star early evolution: the case of the Herschel 36 A triple system

Autores
Arias, Julia Ines; Holgado, Gonzalo; Gamen, Roberto Claudio; Morrell, Nidia Irene; Campillay, Abdo R.
Año de publicación
2024
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Theoretical models show that some massive stars have not yet arrived at the zero-age main sequence (ZAMS) at the end of the accretion phase. At that time, they have lost their thick envelopes and thus could be optically visible. Although some candidates to optically observable ZAMS stars have been reported, the evolutionary status of none of them has been confirmed yet. The O-type triple system Herschel 36 A (H36A) is one of these candidates. We present the quantitative spectral analysis of the individual stellar components of H36A and investigate the evolutionary status of the system by contrasting main-sequence and pre-main-sequence models. Overall, the derived parameters suggest that the components of H36A could be pre-main-sequence stars going through the very last contraction to the ZAMS. However, the possibility of them already being on the main sequence is not yet ruled out. This study highlights the importance of considering multiple evolutionary models and shows that H36A represents a key object for understanding massive star formation and early evolution.
Fil: Arias, Julia Ines. 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. Universidad de La Serena; Chile
Fil: Holgado, Gonzalo. Instituto de Astrofísica de Canarias; España
Fil: Gamen, Roberto Claudio. 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
Fil: Morrell, Nidia Irene. 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. Observatorio Las Campanas; Chile
Fil: Campillay, Abdo R.. Universidad de La Serena; Chile
Materia
Stars: binaries: close
Stars: binaries: spectroscopic
Stars: individual: Herschel 36
Stars: massive
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/257174
Acceder
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network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling Exploring massive star early evolution: the case of the Herschel 36 A triple systemArias, Julia InesHolgado, GonzaloGamen, Roberto ClaudioMorrell, Nidia IreneCampillay, Abdo R.Stars: binaries: closeStars: binaries: spectroscopicStars: individual: Herschel 36Stars: massivehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Theoretical models show that some massive stars have not yet arrived at the zero-age main sequence (ZAMS) at the end of the accretion phase. At that time, they have lost their thick envelopes and thus could be optically visible. Although some candidates to optically observable ZAMS stars have been reported, the evolutionary status of none of them has been confirmed yet. The O-type triple system Herschel 36 A (H36A) is one of these candidates. We present the quantitative spectral analysis of the individual stellar components of H36A and investigate the evolutionary status of the system by contrasting main-sequence and pre-main-sequence models. Overall, the derived parameters suggest that the components of H36A could be pre-main-sequence stars going through the very last contraction to the ZAMS. However, the possibility of them already being on the main sequence is not yet ruled out. This study highlights the importance of considering multiple evolutionary models and shows that H36A represents a key object for understanding massive star formation and early evolution.Fil: Arias, Julia Ines. 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. Universidad de La Serena; ChileFil: Holgado, Gonzalo. Instituto de Astrofísica de Canarias; EspañaFil: Gamen, Roberto Claudio. 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; ArgentinaFil: Morrell, Nidia Irene. 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. Observatorio Las Campanas; ChileFil: Campillay, Abdo R.. Universidad de La Serena; ChileWiley Blackwell Publishing, Inc2024-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/257174Arias, Julia Ines; Holgado, Gonzalo; Gamen, Roberto Claudio; Morrell, Nidia Irene; Campillay, Abdo R.; Exploring massive star early evolution: the case of the Herschel 36 A triple system; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 535; 1; 11-2024; 359-3690035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/535/1/359/7821245info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stae2354info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:31:49Zoai:ri.conicet.gov.ar:11336/257174instacron: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:34982025-10-22 11:31:49.733CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Exploring massive star early evolution: the case of the Herschel 36 A triple system
title Exploring massive star early evolution: the case of the Herschel 36 A triple system
spellingShingle Exploring massive star early evolution: the case of the Herschel 36 A triple system
Arias, Julia Ines
Stars: binaries: close
Stars: binaries: spectroscopic
Stars: individual: Herschel 36
Stars: massive
title_short Exploring massive star early evolution: the case of the Herschel 36 A triple system
title_full Exploring massive star early evolution: the case of the Herschel 36 A triple system
title_fullStr Exploring massive star early evolution: the case of the Herschel 36 A triple system
title_full_unstemmed Exploring massive star early evolution: the case of the Herschel 36 A triple system
title_sort Exploring massive star early evolution: the case of the Herschel 36 A triple system
dc.creator.none.fl_str_mv Arias, Julia Ines
Holgado, Gonzalo
Gamen, Roberto Claudio
Morrell, Nidia Irene
Campillay, Abdo R.
author Arias, Julia Ines
author_facet Arias, Julia Ines
Holgado, Gonzalo
Gamen, Roberto Claudio
Morrell, Nidia Irene
Campillay, Abdo R.
author_role author
author2 Holgado, Gonzalo
Gamen, Roberto Claudio
Morrell, Nidia Irene
Campillay, Abdo R.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Stars: binaries: close
Stars: binaries: spectroscopic
Stars: individual: Herschel 36
Stars: massive
topic Stars: binaries: close
Stars: binaries: spectroscopic
Stars: individual: Herschel 36
Stars: massive
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Theoretical models show that some massive stars have not yet arrived at the zero-age main sequence (ZAMS) at the end of the accretion phase. At that time, they have lost their thick envelopes and thus could be optically visible. Although some candidates to optically observable ZAMS stars have been reported, the evolutionary status of none of them has been confirmed yet. The O-type triple system Herschel 36 A (H36A) is one of these candidates. We present the quantitative spectral analysis of the individual stellar components of H36A and investigate the evolutionary status of the system by contrasting main-sequence and pre-main-sequence models. Overall, the derived parameters suggest that the components of H36A could be pre-main-sequence stars going through the very last contraction to the ZAMS. However, the possibility of them already being on the main sequence is not yet ruled out. This study highlights the importance of considering multiple evolutionary models and shows that H36A represents a key object for understanding massive star formation and early evolution.
Fil: Arias, Julia Ines. 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. Universidad de La Serena; Chile
Fil: Holgado, Gonzalo. Instituto de Astrofísica de Canarias; España
Fil: Gamen, Roberto Claudio. 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
Fil: Morrell, Nidia Irene. 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. Observatorio Las Campanas; Chile
Fil: Campillay, Abdo R.. Universidad de La Serena; Chile
description Theoretical models show that some massive stars have not yet arrived at the zero-age main sequence (ZAMS) at the end of the accretion phase. At that time, they have lost their thick envelopes and thus could be optically visible. Although some candidates to optically observable ZAMS stars have been reported, the evolutionary status of none of them has been confirmed yet. The O-type triple system Herschel 36 A (H36A) is one of these candidates. We present the quantitative spectral analysis of the individual stellar components of H36A and investigate the evolutionary status of the system by contrasting main-sequence and pre-main-sequence models. Overall, the derived parameters suggest that the components of H36A could be pre-main-sequence stars going through the very last contraction to the ZAMS. However, the possibility of them already being on the main sequence is not yet ruled out. This study highlights the importance of considering multiple evolutionary models and shows that H36A represents a key object for understanding massive star formation and early evolution.
publishDate 2024
dc.date.none.fl_str_mv 2024-11
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/257174
Arias, Julia Ines; Holgado, Gonzalo; Gamen, Roberto Claudio; Morrell, Nidia Irene; Campillay, Abdo R.; Exploring massive star early evolution: the case of the Herschel 36 A triple system; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 535; 1; 11-2024; 359-369
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/257174
identifier_str_mv Arias, Julia Ines; Holgado, Gonzalo; Gamen, Roberto Claudio; Morrell, Nidia Irene; Campillay, Abdo R.; Exploring massive star early evolution: the case of the Herschel 36 A triple system; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 535; 1; 11-2024; 359-369
0035-8711
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://academic.oup.com/mnras/article/535/1/359/7821245
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stae2354
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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
_version_ 1846781925537087488
score 12.982451

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