The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems.
- Autores
- Maiz Apellaniz, J.; Sota, A; Arias, Julia Ines; Barba, Rodolfo Hector; Walborn, Nolan Revere; Simon Diaz, S.; Negueruela, I.; Marco, A.; Leao, J. R. S.; Herrero, A.; Gamen, Roberto Claudio; Alfaro, E. J.
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- This is the third installment of the Galactic O-Star Spectroscopic Survey (GOSSS), a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ∼ 2500 digital observations selected from the Galactic O-Star Catalog. In this paper, we present 142 additional stellar systems with O stars from both hemispheres, bringing the total of O-type systems published within the project to 590. Among the new objects, there are 20 new O stars. We also identify 11 new double-lined spectroscopic binaries, 6 of which are of O+O type and 5 of O+B type, and an additional new tripled-lined spectroscopic binary of O+O+B type. We also revise some of the previous GOSSS classifications, present some egregious examples of stars erroneously classified as O-type in the past, introduce the use of luminosity class IV at spectral types O4-O5.5, and adapt the classification scheme to the work of Arias et al.The GOSSS spectroscopic data in this article were gathered with five facilities: the 1.5 m Telescope at the Observatorio de Sierra Nevada (OSN), the 2.5 m du Pont Telescope at Las Campanas Observatory (LCO), the 3.5 m Telescope at Calar Alto Observatory (CAHA), and the 4.2 m William Herschel Telescope (WHT) and 10.4 m Gran Telescopio Canarias (GTC) at Observatorio del Roque de los Muchachos (ORM).
Fil: Maiz Apellaniz, J.. Consejo Superior de Investigaciones Científicas. Centro de Astrobiología; España
Fil: Sota, A. Instituto de Astrofisica de Andalucia; España
Fil: Arias, Julia Ines. Universidad de la Serena; Chile
Fil: Barba, Rodolfo Hector. Universidad de la Serena; Chile
Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados Unidos
Fil: Simon Diaz, S.. Instituto de Astrofísica de Canarias; España
Fil: Negueruela, I.. Universidad de Alicante; España
Fil: Marco, A.. Universidad de Alicante; España
Fil: Leao, J. R. S.. Universidade Federal do Rio Grande do Norte; Brasil
Fil: Herrero, A.. 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: Alfaro, E. J.. Instituto de Astrofisica de Andalucia; España - Materia
-
Spectroscopic binaries
Visual binaries
Early type stars
Surveys
Emission lines
Be stars - 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:11336/35924
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The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems.Maiz Apellaniz, J.Sota, AArias, Julia InesBarba, Rodolfo HectorWalborn, Nolan RevereSimon Diaz, S.Negueruela, I.Marco, A.Leao, J. R. S.Herrero, A.Gamen, Roberto ClaudioAlfaro, E. J.Spectroscopic binariesVisual binariesEarly type starsSurveysEmission linesBe starshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1This is the third installment of the Galactic O-Star Spectroscopic Survey (GOSSS), a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ∼ 2500 digital observations selected from the Galactic O-Star Catalog. In this paper, we present 142 additional stellar systems with O stars from both hemispheres, bringing the total of O-type systems published within the project to 590. Among the new objects, there are 20 new O stars. We also identify 11 new double-lined spectroscopic binaries, 6 of which are of O+O type and 5 of O+B type, and an additional new tripled-lined spectroscopic binary of O+O+B type. We also revise some of the previous GOSSS classifications, present some egregious examples of stars erroneously classified as O-type in the past, introduce the use of luminosity class IV at spectral types O4-O5.5, and adapt the classification scheme to the work of Arias et al.The GOSSS spectroscopic data in this article were gathered with five facilities: the 1.5 m Telescope at the Observatorio de Sierra Nevada (OSN), the 2.5 m du Pont Telescope at Las Campanas Observatory (LCO), the 3.5 m Telescope at Calar Alto Observatory (CAHA), and the 4.2 m William Herschel Telescope (WHT) and 10.4 m Gran Telescopio Canarias (GTC) at Observatorio del Roque de los Muchachos (ORM).Fil: Maiz Apellaniz, J.. Consejo Superior de Investigaciones Científicas. Centro de Astrobiología; EspañaFil: Sota, A. Instituto de Astrofisica de Andalucia; EspañaFil: Arias, Julia Ines. Universidad de la Serena; ChileFil: Barba, Rodolfo Hector. Universidad de la Serena; ChileFil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados UnidosFil: Simon Diaz, S.. Instituto de Astrofísica de Canarias; EspañaFil: Negueruela, I.. Universidad de Alicante; EspañaFil: Marco, A.. Universidad de Alicante; EspañaFil: Leao, J. R. S.. Universidade Federal do Rio Grande do Norte; BrasilFil: Herrero, A.. 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: Alfaro, E. J.. Instituto de Astrofisica de Andalucia; EspañaIOP Publishing2016-04info: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/11336/35924Maiz Apellaniz, J.; Sota, A; Arias, Julia Ines; Barba, Rodolfo Hector; Walborn, Nolan Revere; et al.; The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems.; IOP Publishing; Astrophysical Journal Supplement Series; 224; 1; 4-2016; 4-450067-0049CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0067-0049/224/1/4/metainfo:eu-repo/semantics/altIdentifier/doi/10.3847/0067-0049/224/1/4info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:28:06Zoai:ri.conicet.gov.ar:11336/35924instacron: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 10:28:07.023CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. |
title |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. |
spellingShingle |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. Maiz Apellaniz, J. Spectroscopic binaries Visual binaries Early type stars Surveys Emission lines Be stars |
title_short |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. |
title_full |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. |
title_fullStr |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. |
title_full_unstemmed |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. |
title_sort |
The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems. |
dc.creator.none.fl_str_mv |
Maiz Apellaniz, J. Sota, A Arias, Julia Ines Barba, Rodolfo Hector Walborn, Nolan Revere Simon Diaz, S. Negueruela, I. Marco, A. Leao, J. R. S. Herrero, A. Gamen, Roberto Claudio Alfaro, E. J. |
author |
Maiz Apellaniz, J. |
author_facet |
Maiz Apellaniz, J. Sota, A Arias, Julia Ines Barba, Rodolfo Hector Walborn, Nolan Revere Simon Diaz, S. Negueruela, I. Marco, A. Leao, J. R. S. Herrero, A. Gamen, Roberto Claudio Alfaro, E. J. |
author_role |
author |
author2 |
Sota, A Arias, Julia Ines Barba, Rodolfo Hector Walborn, Nolan Revere Simon Diaz, S. Negueruela, I. Marco, A. Leao, J. R. S. Herrero, A. Gamen, Roberto Claudio Alfaro, E. J. |
author2_role |
author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Spectroscopic binaries Visual binaries Early type stars Surveys Emission lines Be stars |
topic |
Spectroscopic binaries Visual binaries Early type stars Surveys Emission lines Be 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 |
This is the third installment of the Galactic O-Star Spectroscopic Survey (GOSSS), a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ∼ 2500 digital observations selected from the Galactic O-Star Catalog. In this paper, we present 142 additional stellar systems with O stars from both hemispheres, bringing the total of O-type systems published within the project to 590. Among the new objects, there are 20 new O stars. We also identify 11 new double-lined spectroscopic binaries, 6 of which are of O+O type and 5 of O+B type, and an additional new tripled-lined spectroscopic binary of O+O+B type. We also revise some of the previous GOSSS classifications, present some egregious examples of stars erroneously classified as O-type in the past, introduce the use of luminosity class IV at spectral types O4-O5.5, and adapt the classification scheme to the work of Arias et al.The GOSSS spectroscopic data in this article were gathered with five facilities: the 1.5 m Telescope at the Observatorio de Sierra Nevada (OSN), the 2.5 m du Pont Telescope at Las Campanas Observatory (LCO), the 3.5 m Telescope at Calar Alto Observatory (CAHA), and the 4.2 m William Herschel Telescope (WHT) and 10.4 m Gran Telescopio Canarias (GTC) at Observatorio del Roque de los Muchachos (ORM). Fil: Maiz Apellaniz, J.. Consejo Superior de Investigaciones Científicas. Centro de Astrobiología; España Fil: Sota, A. Instituto de Astrofisica de Andalucia; España Fil: Arias, Julia Ines. Universidad de la Serena; Chile Fil: Barba, Rodolfo Hector. Universidad de la Serena; Chile Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados Unidos Fil: Simon Diaz, S.. Instituto de Astrofísica de Canarias; España Fil: Negueruela, I.. Universidad de Alicante; España Fil: Marco, A.. Universidad de Alicante; España Fil: Leao, J. R. S.. Universidade Federal do Rio Grande do Norte; Brasil Fil: Herrero, A.. 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: Alfaro, E. J.. Instituto de Astrofisica de Andalucia; España |
description |
This is the third installment of the Galactic O-Star Spectroscopic Survey (GOSSS), a massive spectroscopic survey of Galactic O stars, based on new homogeneous, high signal-to-noise ratio, R ∼ 2500 digital observations selected from the Galactic O-Star Catalog. In this paper, we present 142 additional stellar systems with O stars from both hemispheres, bringing the total of O-type systems published within the project to 590. Among the new objects, there are 20 new O stars. We also identify 11 new double-lined spectroscopic binaries, 6 of which are of O+O type and 5 of O+B type, and an additional new tripled-lined spectroscopic binary of O+O+B type. We also revise some of the previous GOSSS classifications, present some egregious examples of stars erroneously classified as O-type in the past, introduce the use of luminosity class IV at spectral types O4-O5.5, and adapt the classification scheme to the work of Arias et al.The GOSSS spectroscopic data in this article were gathered with five facilities: the 1.5 m Telescope at the Observatorio de Sierra Nevada (OSN), the 2.5 m du Pont Telescope at Las Campanas Observatory (LCO), the 3.5 m Telescope at Calar Alto Observatory (CAHA), and the 4.2 m William Herschel Telescope (WHT) and 10.4 m Gran Telescopio Canarias (GTC) at Observatorio del Roque de los Muchachos (ORM). |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-04 |
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/11336/35924 Maiz Apellaniz, J.; Sota, A; Arias, Julia Ines; Barba, Rodolfo Hector; Walborn, Nolan Revere; et al.; The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems.; IOP Publishing; Astrophysical Journal Supplement Series; 224; 1; 4-2016; 4-45 0067-0049 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/35924 |
identifier_str_mv |
Maiz Apellaniz, J.; Sota, A; Arias, Julia Ines; Barba, Rodolfo Hector; Walborn, Nolan Revere; et al.; The galactic O-star Spectroscopic Survey (GOSSS), III : 142 additional O-type systems.; IOP Publishing; Astrophysical Journal Supplement Series; 224; 1; 4-2016; 4-45 0067-0049 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0067-0049/224/1/4/meta info:eu-repo/semantics/altIdentifier/doi/10.3847/0067-0049/224/1/4 |
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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13.070432 |