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
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/86512

id SEDICI_1f0ddc0da3b0b9732971870d10904e78
oai_identifier_str oai:sedici.unlp.edu.ar:10915/86512
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling 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
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
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_ 1844616040348123136
score 13.070432