Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A
- Autores
- Ansín, Tomás; Gamen, Roberto Claudio; Morrell, Nidia Irene; Barba, Rodolfo Héctor; Maíz Apellániz, Jesús; Arias, J. I.; Simón Díaz, S.; Holgado, G.
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The evolution of massive stars is not completely understood. Several phenomena affect their birth, life, and death, multiplicity being one of them. In this context, the OWN and MONOS projects are systematically observing O- and WN-type stars whose multiplicity status is unknown. Their major goal considers the necessity of determining absolute parameters of massive stars. We have collected spectra of HD 93249 A and ALS 12502 A aiming at characterizing their binary nature. For both stars, we analysed high-resolution spectra and combined them with Transiting Exoplanet Survey Satellite (TESS) observations to be compared with binary models constructed by means of the PHOEBE code. We discovered that the radial velocity of HD 93249 A varies with a period of 2.97968 ± 0.00001 d and that the system presents ellipsoidal light variations. We disentangled the composite spectra and classified its components as O9 III and B1.5 III, respectively. Confirmed as a spectroscopic binary, HD 93249 A can no longer be used as spectral classification standard. ALS 12502 A turned out to be a detached eclipsing binary in the TESS and Gaia data. These results enable us to determine absolute parameters for each component in the system.
Fil: Ansín, Tomás. 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: 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. Observatorio Las Campanas, Carnegie Institution; Chile
Fil: Barba, Rodolfo Héctor. Universidad de La Serena; Chile
Fil: Maíz Apellániz, Jesús. CSIC-inta. Centro de Astrobiología; España
Fil: Arias, J. I.. Universidad de La Serena; Chile
Fil: Simón Díaz, S.. Instituto de Astrofísica de Canarias; España
Fil: Holgado, G.. Instituto de Astrofísica de Canarias; España - Materia
-
binaries: spectroscopic
stars: early-type
stars: fundamental parameters
stars: individual: (HD 93249 A); (ALS 12502 A) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/235659
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oai:ri.conicet.gov.ar:11336/235659 |
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spelling |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 AAnsín, TomásGamen, Roberto ClaudioMorrell, Nidia IreneBarba, Rodolfo HéctorMaíz Apellániz, JesúsArias, J. I.Simón Díaz, S.Holgado, G.binaries: spectroscopicstars: early-typestars: fundamental parametersstars: individual: (HD 93249 A); (ALS 12502 A)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The evolution of massive stars is not completely understood. Several phenomena affect their birth, life, and death, multiplicity being one of them. In this context, the OWN and MONOS projects are systematically observing O- and WN-type stars whose multiplicity status is unknown. Their major goal considers the necessity of determining absolute parameters of massive stars. We have collected spectra of HD 93249 A and ALS 12502 A aiming at characterizing their binary nature. For both stars, we analysed high-resolution spectra and combined them with Transiting Exoplanet Survey Satellite (TESS) observations to be compared with binary models constructed by means of the PHOEBE code. We discovered that the radial velocity of HD 93249 A varies with a period of 2.97968 ± 0.00001 d and that the system presents ellipsoidal light variations. We disentangled the composite spectra and classified its components as O9 III and B1.5 III, respectively. Confirmed as a spectroscopic binary, HD 93249 A can no longer be used as spectral classification standard. ALS 12502 A turned out to be a detached eclipsing binary in the TESS and Gaia data. These results enable us to determine absolute parameters for each component in the system.Fil: Ansín, Tomás. 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: 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. Observatorio Las Campanas, Carnegie Institution; ChileFil: Barba, Rodolfo Héctor. Universidad de La Serena; ChileFil: Maíz Apellániz, Jesús. CSIC-inta. Centro de Astrobiología; EspañaFil: Arias, J. I.. Universidad de La Serena; ChileFil: Simón Díaz, S.. Instituto de Astrofísica de Canarias; EspañaFil: Holgado, G.. Instituto de Astrofísica de Canarias; EspañaWiley Blackwell Publishing, Inc2023-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/235659Ansín, Tomás; Gamen, Roberto Claudio; Morrell, Nidia Irene; Barba, Rodolfo Héctor; Maíz Apellániz, Jesús; et al.; Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 525; 3; 11-2023; 4566-45800035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/525/3/4566/7257561info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad2501info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:56:10Zoai:ri.conicet.gov.ar:11336/235659instacron: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 09:56:10.619CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A |
title |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A |
spellingShingle |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A Ansín, Tomás binaries: spectroscopic stars: early-type stars: fundamental parameters stars: individual: (HD 93249 A); (ALS 12502 A) |
title_short |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A |
title_full |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A |
title_fullStr |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A |
title_full_unstemmed |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A |
title_sort |
Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A |
dc.creator.none.fl_str_mv |
Ansín, Tomás Gamen, Roberto Claudio Morrell, Nidia Irene Barba, Rodolfo Héctor Maíz Apellániz, Jesús Arias, J. I. Simón Díaz, S. Holgado, G. |
author |
Ansín, Tomás |
author_facet |
Ansín, Tomás Gamen, Roberto Claudio Morrell, Nidia Irene Barba, Rodolfo Héctor Maíz Apellániz, Jesús Arias, J. I. Simón Díaz, S. Holgado, G. |
author_role |
author |
author2 |
Gamen, Roberto Claudio Morrell, Nidia Irene Barba, Rodolfo Héctor Maíz Apellániz, Jesús Arias, J. I. Simón Díaz, S. Holgado, G. |
author2_role |
author author author author author author author |
dc.subject.none.fl_str_mv |
binaries: spectroscopic stars: early-type stars: fundamental parameters stars: individual: (HD 93249 A); (ALS 12502 A) |
topic |
binaries: spectroscopic stars: early-type stars: fundamental parameters stars: individual: (HD 93249 A); (ALS 12502 A) |
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 evolution of massive stars is not completely understood. Several phenomena affect their birth, life, and death, multiplicity being one of them. In this context, the OWN and MONOS projects are systematically observing O- and WN-type stars whose multiplicity status is unknown. Their major goal considers the necessity of determining absolute parameters of massive stars. We have collected spectra of HD 93249 A and ALS 12502 A aiming at characterizing their binary nature. For both stars, we analysed high-resolution spectra and combined them with Transiting Exoplanet Survey Satellite (TESS) observations to be compared with binary models constructed by means of the PHOEBE code. We discovered that the radial velocity of HD 93249 A varies with a period of 2.97968 ± 0.00001 d and that the system presents ellipsoidal light variations. We disentangled the composite spectra and classified its components as O9 III and B1.5 III, respectively. Confirmed as a spectroscopic binary, HD 93249 A can no longer be used as spectral classification standard. ALS 12502 A turned out to be a detached eclipsing binary in the TESS and Gaia data. These results enable us to determine absolute parameters for each component in the system. Fil: Ansín, Tomás. 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: 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. Observatorio Las Campanas, Carnegie Institution; Chile Fil: Barba, Rodolfo Héctor. Universidad de La Serena; Chile Fil: Maíz Apellániz, Jesús. CSIC-inta. Centro de Astrobiología; España Fil: Arias, J. I.. Universidad de La Serena; Chile Fil: Simón Díaz, S.. Instituto de Astrofísica de Canarias; España Fil: Holgado, G.. Instituto de Astrofísica de Canarias; España |
description |
The evolution of massive stars is not completely understood. Several phenomena affect their birth, life, and death, multiplicity being one of them. In this context, the OWN and MONOS projects are systematically observing O- and WN-type stars whose multiplicity status is unknown. Their major goal considers the necessity of determining absolute parameters of massive stars. We have collected spectra of HD 93249 A and ALS 12502 A aiming at characterizing their binary nature. For both stars, we analysed high-resolution spectra and combined them with Transiting Exoplanet Survey Satellite (TESS) observations to be compared with binary models constructed by means of the PHOEBE code. We discovered that the radial velocity of HD 93249 A varies with a period of 2.97968 ± 0.00001 d and that the system presents ellipsoidal light variations. We disentangled the composite spectra and classified its components as O9 III and B1.5 III, respectively. Confirmed as a spectroscopic binary, HD 93249 A can no longer be used as spectral classification standard. ALS 12502 A turned out to be a detached eclipsing binary in the TESS and Gaia data. These results enable us to determine absolute parameters for each component in the system. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-11 |
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/11336/235659 Ansín, Tomás; Gamen, Roberto Claudio; Morrell, Nidia Irene; Barba, Rodolfo Héctor; Maíz Apellániz, Jesús; et al.; Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 525; 3; 11-2023; 4566-4580 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/235659 |
identifier_str_mv |
Ansín, Tomás; Gamen, Roberto Claudio; Morrell, Nidia Irene; Barba, Rodolfo Héctor; Maíz Apellániz, Jesús; et al.; Fundamental parameters of two O9-type giant stars: the (former) spectral classification standard HD 93249 A and ALS 12502 A; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 525; 3; 11-2023; 4566-4580 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/525/3/4566/7257561 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad2501 |
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.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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1844613689131401216 |
score |
13.070432 |