About: Multiwavelength spectroscopy: a diagnostic tool for stellar winds and mass loss application to Be stars

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Attributs	Valeurs
type	work Article
Is Part Of	Evolution of Massive Stars, Mass Loss and Winds
Title	Multiwavelength spectroscopy: a diagnostic tool for stellar winds and mass loss application to Be stars
Date	2004-01-01(xsd:dateTime)
has manifestation of work	http://hub.abes.fr/edp/periodical/eas/2004/volume_13/issue_2004/eas13013/m/web http://hub.abes.fr/edp/periodical/eas/2004/volume_13/issue_2004/eas13013/m/print
related by	http://hub.abes.fr/edp/periodical/eas/2004/volume_13/issue_2004/eas13013/authorship/1 http://hub.abes.fr/edp/periodical/eas/2004/volume_13/issue_2004/eas13013/authorship/2 http://hub.abes.fr/edp/periodical/eas/2004/volume_13/issue_2004/eas13013/authorship/3 http://hub.abes.fr/edp/periodical/eas/2004/volume_13/issue_2004/eas13013/authorship/4
Author	Neiner, C.
Editor	Heydari-Malayeri, M. Stee, Ph. Zahn, J.-P.
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.
article type	research-article
publisher identifier	eas13013
Date Copyrighted	2004-01-01(xsd:dateTime)
Rights	© EAS, EDP Sciences, 2004
Rights Holder	EAS, EDP Sciences
is part of this journal	EAS Publications Series
is primary topic of	http://hub.abes.fr/edp/periodical/eas/2004/volume_13/issue_2004/eas13013/w/record

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