The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars

Autores
Sota, A.; Maíz Apellaniz, J.; Morrell, Nidia Irene; Barba, Rodolfo Hector; Walborn, Nolan R.; Gamen, Roberto Claudio; Arias, J. I.; Alfaro, E. J.
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present the second installment of GOSSS, a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ~ 2500 digital observations from both hemispheres selected from the Galactic O-Star Catalog (GOSC). In this paper we include bright stars and other objects drawn mostly from the first version of GOSC, all of them south of δ = ?20°, for a total number of 258 O stars. We also revise the northern sample of Paper I to provide the full list of spectroscopically classified Galactic O stars complete to B = 8, bringing the total number of published GOSSS stars to 448. Extensive sequences of exceptional objects are given, including the early Of/WN, O Iafpe, Ofc, ON/OC, Onfp, Of?p, and Oe types, as well as double/triple-lined spectroscopic binaries. The new spectral subtype O9.2 is also discussed. The magnitude and spatial distributions of the observed sample are analyzed. We also present new results from OWN, a multi-epoch high-resolution spectroscopic survey coordinated with GOSSS that is assembling the largest sample of Galactic spectroscopic massive binaries ever attained. The OWN data combined with additional information on spectroscopic and visual binaries from the literature indicate that only a very small fraction (if any) of the stars with masses above 15-20 M ☉ are born as single systems. In the future we will publish the rest of the GOSSS survey, which is expected to include over 1000 Galactic O stars.
Fil: Sota, A.. Instituto de Astrofísica de Andalucía. CSIC; España
Fil: Maíz Apellaniz, J.. Instituto de Astrofísica de Andalucía. CSIC; España
Fil: Morrell, Nidia Irene. Las Campanas Observatory. Carnegie Observatories; Chile
Fil: Barba, Rodolfo Hector. Universidad de la Serena; Chile
Fil: Walborn, Nolan R.. Space Telescope Science Institute; Estados Unidos
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: Arias, J. I.. Las Campanas Observatory. Carnegie Observatories; Chile
Fil: Alfaro, E. J.. Instituto de Astrofísica de Andalucía. CSIC; España
Materia
Binaries
Early type stars
Spectroscopy
Emission line stars
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/15547
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/15547
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern starsSota, A.Maíz Apellaniz, J.Morrell, Nidia IreneBarba, Rodolfo HectorWalborn, Nolan R.Gamen, Roberto ClaudioArias, J. I.Alfaro, E. J.BinariesEarly type starsSpectroscopyEmission line starshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the second installment of GOSSS, a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ~ 2500 digital observations from both hemispheres selected from the Galactic O-Star Catalog (GOSC). In this paper we include bright stars and other objects drawn mostly from the first version of GOSC, all of them south of δ = ?20°, for a total number of 258 O stars. We also revise the northern sample of Paper I to provide the full list of spectroscopically classified Galactic O stars complete to B = 8, bringing the total number of published GOSSS stars to 448. Extensive sequences of exceptional objects are given, including the early Of/WN, O Iafpe, Ofc, ON/OC, Onfp, Of?p, and Oe types, as well as double/triple-lined spectroscopic binaries. The new spectral subtype O9.2 is also discussed. The magnitude and spatial distributions of the observed sample are analyzed. We also present new results from OWN, a multi-epoch high-resolution spectroscopic survey coordinated with GOSSS that is assembling the largest sample of Galactic spectroscopic massive binaries ever attained. The OWN data combined with additional information on spectroscopic and visual binaries from the literature indicate that only a very small fraction (if any) of the stars with masses above 15-20 M ☉ are born as single systems. In the future we will publish the rest of the GOSSS survey, which is expected to include over 1000 Galactic O stars.Fil: Sota, A.. Instituto de Astrofísica de Andalucía. CSIC; EspañaFil: Maíz Apellaniz, J.. Instituto de Astrofísica de Andalucía. CSIC; EspañaFil: Morrell, Nidia Irene. Las Campanas Observatory. Carnegie Observatories; ChileFil: Barba, Rodolfo Hector. Universidad de la Serena; ChileFil: Walborn, Nolan R.. Space Telescope Science Institute; Estados UnidosFil: 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: Arias, J. I.. Las Campanas Observatory. Carnegie Observatories; ChileFil: Alfaro, E. J.. Instituto de Astrofísica de Andalucía. CSIC; EspañaIop Publishing2014-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/15547Sota, A.; Maíz Apellaniz, J.; Morrell, Nidia Irene; Barba, Rodolfo Hector; Walborn, Nolan R.; et al.; The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars; Iop Publishing; Astrophysical Journal Supplement Series; 211; 1; 3-2014; 10-930067-0049enginfo:eu-repo/semantics/altIdentifier/doi/10.1088/0067-0049/211/1/10info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0067-0049/211/1/10/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:57:42Zoai:ri.conicet.gov.ar:11336/15547instacron: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 09:57:42.847CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
title The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
spellingShingle The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
Sota, A.
Binaries
Early type stars
Spectroscopy
Emission line stars
title_short The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
title_full The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
title_fullStr The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
title_full_unstemmed The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
title_sort The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars
dc.creator.none.fl_str_mv Sota, A.
Maíz Apellaniz, J.
Morrell, Nidia Irene
Barba, Rodolfo Hector
Walborn, Nolan R.
Gamen, Roberto Claudio
Arias, J. I.
Alfaro, E. J.
author Sota, A.
author_facet Sota, A.
Maíz Apellaniz, J.
Morrell, Nidia Irene
Barba, Rodolfo Hector
Walborn, Nolan R.
Gamen, Roberto Claudio
Arias, J. I.
Alfaro, E. J.
author_role author
author2 Maíz Apellaniz, J.
Morrell, Nidia Irene
Barba, Rodolfo Hector
Walborn, Nolan R.
Gamen, Roberto Claudio
Arias, J. I.
Alfaro, E. J.
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Binaries
Early type stars
Spectroscopy
Emission line stars
topic Binaries
Early type stars
Spectroscopy
Emission line stars
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present the second installment of GOSSS, a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ~ 2500 digital observations from both hemispheres selected from the Galactic O-Star Catalog (GOSC). In this paper we include bright stars and other objects drawn mostly from the first version of GOSC, all of them south of δ = ?20°, for a total number of 258 O stars. We also revise the northern sample of Paper I to provide the full list of spectroscopically classified Galactic O stars complete to B = 8, bringing the total number of published GOSSS stars to 448. Extensive sequences of exceptional objects are given, including the early Of/WN, O Iafpe, Ofc, ON/OC, Onfp, Of?p, and Oe types, as well as double/triple-lined spectroscopic binaries. The new spectral subtype O9.2 is also discussed. The magnitude and spatial distributions of the observed sample are analyzed. We also present new results from OWN, a multi-epoch high-resolution spectroscopic survey coordinated with GOSSS that is assembling the largest sample of Galactic spectroscopic massive binaries ever attained. The OWN data combined with additional information on spectroscopic and visual binaries from the literature indicate that only a very small fraction (if any) of the stars with masses above 15-20 M ☉ are born as single systems. In the future we will publish the rest of the GOSSS survey, which is expected to include over 1000 Galactic O stars.
Fil: Sota, A.. Instituto de Astrofísica de Andalucía. CSIC; España
Fil: Maíz Apellaniz, J.. Instituto de Astrofísica de Andalucía. CSIC; España
Fil: Morrell, Nidia Irene. Las Campanas Observatory. Carnegie Observatories; Chile
Fil: Barba, Rodolfo Hector. Universidad de la Serena; Chile
Fil: Walborn, Nolan R.. Space Telescope Science Institute; Estados Unidos
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: Arias, J. I.. Las Campanas Observatory. Carnegie Observatories; Chile
Fil: Alfaro, E. J.. Instituto de Astrofísica de Andalucía. CSIC; España
description We present the second installment of GOSSS, a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ~ 2500 digital observations from both hemispheres selected from the Galactic O-Star Catalog (GOSC). In this paper we include bright stars and other objects drawn mostly from the first version of GOSC, all of them south of δ = ?20°, for a total number of 258 O stars. We also revise the northern sample of Paper I to provide the full list of spectroscopically classified Galactic O stars complete to B = 8, bringing the total number of published GOSSS stars to 448. Extensive sequences of exceptional objects are given, including the early Of/WN, O Iafpe, Ofc, ON/OC, Onfp, Of?p, and Oe types, as well as double/triple-lined spectroscopic binaries. The new spectral subtype O9.2 is also discussed. The magnitude and spatial distributions of the observed sample are analyzed. We also present new results from OWN, a multi-epoch high-resolution spectroscopic survey coordinated with GOSSS that is assembling the largest sample of Galactic spectroscopic massive binaries ever attained. The OWN data combined with additional information on spectroscopic and visual binaries from the literature indicate that only a very small fraction (if any) of the stars with masses above 15-20 M ☉ are born as single systems. In the future we will publish the rest of the GOSSS survey, which is expected to include over 1000 Galactic O stars.
publishDate 2014
dc.date.none.fl_str_mv 2014-03
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/11336/15547
Sota, A.; Maíz Apellaniz, J.; Morrell, Nidia Irene; Barba, Rodolfo Hector; Walborn, Nolan R.; et al.; The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars; Iop Publishing; Astrophysical Journal Supplement Series; 211; 1; 3-2014; 10-93
0067-0049
url http://hdl.handle.net/11336/15547
identifier_str_mv Sota, A.; Maíz Apellaniz, J.; Morrell, Nidia Irene; Barba, Rodolfo Hector; Walborn, Nolan R.; et al.; The Galactic O-Star Spectroscopic Survey (GOSSS). II : bright southern stars; Iop Publishing; Astrophysical Journal Supplement Series; 211; 1; 3-2014; 10-93
0067-0049
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1088/0067-0049/211/1/10
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0067-0049/211/1/10/meta
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
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing
publisher.none.fl_str_mv Iop Publishing
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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score 13.070432

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