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
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/83142
Acceder
id SEDICI_019939c1f8efa22949f1b873ea0c6cc6
oai_identifier_str oai:sedici.unlp.edu.ar:10915/83142
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling 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:UNLP2025-10-22T16:56:33Zoai: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:13292025-10-22 16:56:33.29SEDICI (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
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
_version_ 1846783172366303232
score 12.982451

Publicaciones similares