Pismis 24-1: The stellar upper mass limit preserved
- Autores
- Maíz Apellániz, Jesús; Walborn, Nolan Revere; Morrell, Nidia Irene; Niemelä, Virpi Sinikka; Nelan, E. P.
- Año de publicación
- 2007
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Is there a stellar upper mass limit? Recent statistical work seems to indicate that there is and that it is in the vicinity of 150 M⊙. In this paper we use HST and ground-based data to investigate the brightest members of the cluster Pismis 24, one of which (Pismis 24-1) was previously inferred to have a mass greater than 200 M⊙, in apparent disagreement with that limit. We determine that Pismis 24-1 is composed of at least three objects, the resolved Pismis 24-1SW and the unresolved spectroscopic binary Pismis 24-1NE. The evolutionary zero-age masses of Pismis 24-1SW, the unresolved system Pismis 24-1NE, and the nearby star Pismis 24-17 are all ≈100 Mȯ, very large but under the stellar upper mass limit.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Binaries: close
Stars: early-type
Stars: Fundamental parameters
Stars: individual (Pismis 24-17, Pismis 24-1NW, Pismis 24-1SE) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/83142
Ver los metadatos del registro completo
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Pismis 24-1: The stellar upper mass limit preservedMaíz Apellániz, JesúsWalborn, Nolan RevereMorrell, Nidia IreneNiemelä, Virpi SinikkaNelan, E. P.Ciencias AstronómicasBinaries: closeStars: early-typeStars: Fundamental parametersStars: individual (Pismis 24-17, Pismis 24-1NW, Pismis 24-1SE)Is there a stellar upper mass limit? Recent statistical work seems to indicate that there is and that it is in the vicinity of 150 M⊙. In this paper we use HST and ground-based data to investigate the brightest members of the cluster Pismis 24, one of which (Pismis 24-1) was previously inferred to have a mass greater than 200 M⊙, in apparent disagreement with that limit. We determine that Pismis 24-1 is composed of at least three objects, the resolved Pismis 24-1SW and the unresolved spectroscopic binary Pismis 24-1NE. The evolutionary zero-age masses of Pismis 24-1SW, the unresolved system Pismis 24-1NE, and the nearby star Pismis 24-17 are all ≈100 Mȯ, very large but under the stellar upper mass limit.Facultad de Ciencias Astronómicas y Geofísicas2007-05-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1480-1485http://sedici.unlp.edu.ar/handle/10915/83142enginfo:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/altIdentifier/doi/10.1086/513098info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:15:41Zoai:sedici.unlp.edu.ar:10915/83142Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:42.169SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Pismis 24-1: The stellar upper mass limit preserved |
title |
Pismis 24-1: The stellar upper mass limit preserved |
spellingShingle |
Pismis 24-1: The stellar upper mass limit preserved Maíz Apellániz, Jesús Ciencias Astronómicas Binaries: close Stars: early-type Stars: Fundamental parameters Stars: individual (Pismis 24-17, Pismis 24-1NW, Pismis 24-1SE) |
title_short |
Pismis 24-1: The stellar upper mass limit preserved |
title_full |
Pismis 24-1: The stellar upper mass limit preserved |
title_fullStr |
Pismis 24-1: The stellar upper mass limit preserved |
title_full_unstemmed |
Pismis 24-1: The stellar upper mass limit preserved |
title_sort |
Pismis 24-1: The stellar upper mass limit preserved |
dc.creator.none.fl_str_mv |
Maíz Apellániz, Jesús Walborn, Nolan Revere Morrell, Nidia Irene Niemelä, Virpi Sinikka Nelan, E. P. |
author |
Maíz Apellániz, Jesús |
author_facet |
Maíz Apellániz, Jesús Walborn, Nolan Revere Morrell, Nidia Irene Niemelä, Virpi Sinikka Nelan, E. P. |
author_role |
author |
author2 |
Walborn, Nolan Revere Morrell, Nidia Irene Niemelä, Virpi Sinikka Nelan, E. P. |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Binaries: close Stars: early-type Stars: Fundamental parameters Stars: individual (Pismis 24-17, Pismis 24-1NW, Pismis 24-1SE) |
topic |
Ciencias Astronómicas Binaries: close Stars: early-type Stars: Fundamental parameters Stars: individual (Pismis 24-17, Pismis 24-1NW, Pismis 24-1SE) |
dc.description.none.fl_txt_mv |
Is there a stellar upper mass limit? Recent statistical work seems to indicate that there is and that it is in the vicinity of 150 M⊙. In this paper we use HST and ground-based data to investigate the brightest members of the cluster Pismis 24, one of which (Pismis 24-1) was previously inferred to have a mass greater than 200 M⊙, in apparent disagreement with that limit. We determine that Pismis 24-1 is composed of at least three objects, the resolved Pismis 24-1SW and the unresolved spectroscopic binary Pismis 24-1NE. The evolutionary zero-age masses of Pismis 24-1SW, the unresolved system Pismis 24-1NE, and the nearby star Pismis 24-17 are all ≈100 Mȯ, very large but under the stellar upper mass limit. Facultad de Ciencias Astronómicas y Geofísicas |
description |
Is there a stellar upper mass limit? Recent statistical work seems to indicate that there is and that it is in the vicinity of 150 M⊙. In this paper we use HST and ground-based data to investigate the brightest members of the cluster Pismis 24, one of which (Pismis 24-1) was previously inferred to have a mass greater than 200 M⊙, in apparent disagreement with that limit. We determine that Pismis 24-1 is composed of at least three objects, the resolved Pismis 24-1SW and the unresolved spectroscopic binary Pismis 24-1NE. The evolutionary zero-age masses of Pismis 24-1SW, the unresolved system Pismis 24-1NE, and the nearby star Pismis 24-17 are all ≈100 Mȯ, very large but under the stellar upper mass limit. |
publishDate |
2007 |
dc.date.none.fl_str_mv |
2007-05-04 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/83142 |
url |
http://sedici.unlp.edu.ar/handle/10915/83142 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-637X info:eu-repo/semantics/altIdentifier/doi/10.1086/513098 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 1480-1485 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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SEDICI (UNLP) |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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