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.
@article{arxiv.1111.1341,
title = {The IACOB project: A grid-based automatic tool for the quantitative spectroscopic analysis of O-stars},
author = {S. Simón-Díaz and N. Castro and A. Herrero and J. Puls and M. Garcia and C. Sabín-Sanjulián},
journal= {arXiv preprint arXiv:1111.1341},
year = {2015}
}
Comments
8 pages, 2 figures, 1 table. Proceedings of the "GREAT-ESF Stellar Atmospheres in the Gaia Era Workshop"