Hostname: page-component-8448b6f56d-t5pn6 Total loading time: 0 Render date: 2024-04-18T02:54:10.789Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Get access

Abstract

Spectroscopy can be used as a tool to study stellar winds and mass-loss. The combination of spectroscopic data at several wavelengths, in particular Ultra-Violet (UV), visible and Infra-Red (IR), provides a complete picture of the stellar environment. In this paper, Be stars are taken as an example for which multiwavelength spectroscopy provides essential information on the stellar 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

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)