ISO impact on stellar models and vice versa
Astrophysics
2007-05-23 v1
Abstract
We present a detailed spectroscopic study of a sample of bright, mostly cool, stars observed with the Short-Wavelength Spectrometer (SWS) on board the Infrared Space Observatory (ISO), which enables the accurate determination of the stellar parameters of the cool giants, but also serves as a critical review of the ISO-SWS calibration.
Cite
@article{arxiv.astro-ph/0008362,
title = {ISO impact on stellar models and vice versa},
author = {L. Decin and C. Waelkens and K. Eriksson and B. Gustafsson and B. Plez and A. J. Sauval and W. Van Assche and B. Vandenbussche},
journal= {arXiv preprint arXiv:astro-ph/0008362},
year = {2007}
}
Comments
6 pages, 3 figures, to appear in `ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy', held 2-4 February 2000, at VILSPA