ISO impact on stellar models and vice versa

(2) Astronomiska Observatoriet; (3) Universite de Montpellier II; (4) Observatoire Royal de Belgique; (5) Instituut voor Wiskunde; A.J. Sauval (4); Belgium; Belgium); B. Gustafsson (2) B.Plez (3); Bruxelles; B. Vandenbussche (1) ((1) Instituut voor Sterrenkunde

arxiv: astro-ph/0008362 · v1 · submitted 2000-08-23 · 🌌 astro-ph

ISO impact on stellar models and vice versa

L. Decin (1) , C. Waelkens (1) , K. Eriksson (2) , B. Gustafsson (2) B.Plez (3) , A.J. Sauval (4) , W. Van Assche (5) , B. Vandenbussche (1) ((1) Instituut voor Sterrenkunde , Leuven

show 11 more authors

Belgium (2) Astronomiska Observatoriet Uppsala Sweden (3) Universite de Montpellier II Montpellier France (4) Observatoire Royal de Belgique Bruxelles (5) Instituut voor Wiskunde Belgium)

This is my paper

classification 🌌 astro-ph

keywords coolstellaraccurateboardbrightcalibrationcriticaldetailed

0 comments

read the original 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.

This paper has not been read by Pith yet.

ISO impact on stellar models and vice versa

discussion (0)