Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS)
- Autores
- Arias, Julia Inés; Walborn, Nolan Revere; Díaz, S. S.; Barbá, Rodolfo Héctor; Maíz Apellániz, Jesús; Sabín Sanjulián, C.; Gamen, Roberto Claudio; Morrell, Nidia Irene; Sota, Alfredo; Marco, A.; Negueruela, I.; Leão, J. R. S.; Herrero, A.; Alfaro, Emilio J.
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- On the basis of the Galactic O Star Spectroscopic Survey (GOSSS), we present a detailed systematic investigation of the O Vz stars. The currently used spectral classification criteria are rediscussed, and the Vz phenomenon is recalibrated through the addition of a quantitative criterion based on the equivalent widths of the He i λ4471, He ii λ4542, and He ii λ4686 spectral lines. The GOSSS O Vz and O V populations resulting from the newly adopted spectral classification criteria are comparatively analyzed. The locations of the O Vz stars are probed, showing a concentration of the most extreme cases toward the youngest star-forming regions. The occurrence of the Vz spectral peculiarity in a solar-metallicity environment, as predicted by the fastwind code, is also investigated, confirming the importance of taking into account several processes for the correct interpretation of the phenomenon.
Instituto de Astrofísica de La Plata
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
stars: early-type
stars: fundamental parameters
surveys - 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:10915/86512
Ver los metadatos del registro completo
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Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS)Arias, Julia InésWalborn, Nolan RevereDíaz, S. S.Barbá, Rodolfo HéctorMaíz Apellániz, JesúsSabín Sanjulián, C.Gamen, Roberto ClaudioMorrell, Nidia IreneSota, AlfredoMarco, A.Negueruela, I.Leão, J. R. S.Herrero, A.Alfaro, Emilio J.Ciencias Astronómicasstars: early-typestars: fundamental parameterssurveysOn the basis of the Galactic O Star Spectroscopic Survey (GOSSS), we present a detailed systematic investigation of the O Vz stars. The currently used spectral classification criteria are rediscussed, and the Vz phenomenon is recalibrated through the addition of a quantitative criterion based on the equivalent widths of the He i λ4471, He ii λ4542, and He ii λ4686 spectral lines. The GOSSS O Vz and O V populations resulting from the newly adopted spectral classification criteria are comparatively analyzed. The locations of the O Vz stars are probed, showing a concentration of the most extreme cases toward the youngest star-forming regions. The occurrence of the Vz spectral peculiarity in a solar-metallicity environment, as predicted by the fastwind code, is also investigated, confirming the importance of taking into account several processes for the correct interpretation of the phenomenon.Instituto de Astrofísica de La PlataFacultad de Ciencias Astronómicas y Geofísicas2016info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/86512enginfo:eu-repo/semantics/altIdentifier/issn/0004-6256info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-6256/152/2/31info: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:UNLP2025-09-29T11:16:45Zoai:sedici.unlp.edu.ar:10915/86512Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:45.383SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) |
title |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) |
spellingShingle |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) Arias, Julia Inés Ciencias Astronómicas stars: early-type stars: fundamental parameters surveys |
title_short |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) |
title_full |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) |
title_fullStr |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) |
title_full_unstemmed |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) |
title_sort |
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS) |
dc.creator.none.fl_str_mv |
Arias, Julia Inés Walborn, Nolan Revere Díaz, S. S. Barbá, Rodolfo Héctor Maíz Apellániz, Jesús Sabín Sanjulián, C. Gamen, Roberto Claudio Morrell, Nidia Irene Sota, Alfredo Marco, A. Negueruela, I. Leão, J. R. S. Herrero, A. Alfaro, Emilio J. |
author |
Arias, Julia Inés |
author_facet |
Arias, Julia Inés Walborn, Nolan Revere Díaz, S. S. Barbá, Rodolfo Héctor Maíz Apellániz, Jesús Sabín Sanjulián, C. Gamen, Roberto Claudio Morrell, Nidia Irene Sota, Alfredo Marco, A. Negueruela, I. Leão, J. R. S. Herrero, A. Alfaro, Emilio J. |
author_role |
author |
author2 |
Walborn, Nolan Revere Díaz, S. S. Barbá, Rodolfo Héctor Maíz Apellániz, Jesús Sabín Sanjulián, C. Gamen, Roberto Claudio Morrell, Nidia Irene Sota, Alfredo Marco, A. Negueruela, I. Leão, J. R. S. Herrero, A. Alfaro, Emilio J. |
author2_role |
author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas stars: early-type stars: fundamental parameters surveys |
topic |
Ciencias Astronómicas stars: early-type stars: fundamental parameters surveys |
dc.description.none.fl_txt_mv |
On the basis of the Galactic O Star Spectroscopic Survey (GOSSS), we present a detailed systematic investigation of the O Vz stars. The currently used spectral classification criteria are rediscussed, and the Vz phenomenon is recalibrated through the addition of a quantitative criterion based on the equivalent widths of the He i λ4471, He ii λ4542, and He ii λ4686 spectral lines. The GOSSS O Vz and O V populations resulting from the newly adopted spectral classification criteria are comparatively analyzed. The locations of the O Vz stars are probed, showing a concentration of the most extreme cases toward the youngest star-forming regions. The occurrence of the Vz spectral peculiarity in a solar-metallicity environment, as predicted by the fastwind code, is also investigated, confirming the importance of taking into account several processes for the correct interpretation of the phenomenon. Instituto de Astrofísica de La Plata Facultad de Ciencias Astronómicas y Geofísicas |
description |
On the basis of the Galactic O Star Spectroscopic Survey (GOSSS), we present a detailed systematic investigation of the O Vz stars. The currently used spectral classification criteria are rediscussed, and the Vz phenomenon is recalibrated through the addition of a quantitative criterion based on the equivalent widths of the He i λ4471, He ii λ4542, and He ii λ4686 spectral lines. The GOSSS O Vz and O V populations resulting from the newly adopted spectral classification criteria are comparatively analyzed. The locations of the O Vz stars are probed, showing a concentration of the most extreme cases toward the youngest star-forming regions. The occurrence of the Vz spectral peculiarity in a solar-metallicity environment, as predicted by the fastwind code, is also investigated, confirming the importance of taking into account several processes for the correct interpretation of the phenomenon. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016 |
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/10915/86512 |
url |
http://sedici.unlp.edu.ar/handle/10915/86512 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6256 info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-6256/152/2/31 |
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 |
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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 |
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