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: | , , , , , , , , , , , , , |
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Formato: | Articulo |
Lenguaje: | Inglés |
Publicado: |
2016
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/86512 |
Aporte de: |
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I19-R120-10915-86512 |
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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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