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Multiwavelength spectroscopy: a diagnostic tool for stellar winds andmass loss application to Be stars

Published online by Cambridge University Press:  15 November 2004

M. Heydari-Malayeri ,
Ph. Stee ,
J.-P. Zahn  and
C. Neiner
C. Neiner*
Affiliation:
RSSD, ESTEC, ESA, Keplerlaan 1, 2201 AZ Noordwijk ZH, Netherlands GEPI, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France
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Abstract

Spectroscopy can be used as a tool to study stellar winds and mass-loss. Thecombination of spectroscopic data at several wavelengths, in particularUltra-Violet (UV), visible and Infra-Red (IR), provides a complete picture ofthe stellar environment. In this paper, Be stars are taken as an example forwhich multiwavelength spectroscopy provides essential information on thestellar wind and mass-loss.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 13: Evolution of Massive Stars, Mass Loss and Winds , 2004 , pp. 339 - 361
Copyright
© EAS, EDP Sciences, 2004

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