Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS)

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...

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Autores principales: 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.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2016
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/86512
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id I19-R120-10915-86512
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
stars: early-type
stars: fundamental parameters
surveys
spellingShingle Ciencias Astronómicas
stars: early-type
stars: fundamental parameters
surveys
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.
Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS)
topic_facet Ciencias Astronómicas
stars: early-type
stars: fundamental parameters
surveys
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.
format Articulo
Articulo
author 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_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_sort Arias, Julia Inés
title Spectral classification and properties of the O VZ stars in the Galactic O-Star Spectroscopic Survey (GOSSS)
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)
publishDate 2016
url http://sedici.unlp.edu.ar/handle/10915/86512
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