The IACOB project: A grid-based automatic tool for the quantitative spectroscopic analysis of O-stars

Bibcode
2011JPhCS.328a2021S
DOI
10.1088/1742-6596/328/1/012021
Simón-Díaz, S.; Castro, N.; Herrero, A.; Puls, J.; Garcia, M.; Sabín-Sanjulián, C.
Referencia bibliográfica

Journal of Physics: Conference Series, Volume 328, Issue 1, pp. 012021 (2011).

Fecha de publicación:
12
2011
Número de autores
6
Número de autores del IAC
0
Número de citas
24
Número de citas referidas
20
Descripción
We present the IACOB grid-based automatic tool for the quantitative spectroscopic analysis of O-stars. The tool consists of an extensive grid of FASTWIND models, and a variety of programs implemented in IDL to handle the observations, perform the automatic analysis, and visualize the results. The tool provides a fast and objective way to determine the stellar parameters and the associated uncertainties of large samples of O-type stars within a reasonable computational time.
Tipo
Sin árbitro

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