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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/257174
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:02:21Zoai: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:34982025-09-29 10:02:22.191CONICET 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 |
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1844613827160702976 |
score |
13.070432 |