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

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

2011-11-05

arxiv.org/abs/1111.1341v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

8 pages, 2 figures, 1 table. Proceedings of the "GREAT-ESF Stellar Atmospheres in the Gaia Era Workshop"

Scientific paper

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.

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