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Attributs	Valeurs
type	work Article
Is Part Of	Low-Mass Stars and the Transition Stars/Brown Dwarfs - Evry Schatzman School on Stellar Physics XXIII
Title	Metallicity
has manifestation of work	http://hub.abes.fr/edp/periodical/eas/2012/volume_57/issue_2012/eas1257006/m/print http://hub.abes.fr/edp/periodical/eas/2012/volume_57/issue_2012/eas1257006/m/web
related by	http://hub.abes.fr/edp/periodical/eas/2012/volume_57/issue_2012/eas1257006/authorship/3 http://hub.abes.fr/edp/periodical/eas/2012/volume_57/issue_2012/eas1257006/authorship/1 http://hub.abes.fr/edp/periodical/eas/2012/volume_57/issue_2012/eas1257006/authorship/4 http://hub.abes.fr/edp/periodical/eas/2012/volume_57/issue_2012/eas1257006/authorship/2
Author	Bonfils X.
Editor	Schultheis M. Reylé C. Charbonnel C.
Abstract	The metallicity measures the fraction of the star that is made of elements heavier than helium. It is intimately related to the stellar structure and composition and thus plays an important role in a broad range of astrophysical cases, from stellar populations to planet formation. This chapter aims to review the recent observational efforts to measure the metallicity of M dwarfs and to screen few astrophysical cases which have benefited from quantitative metallicity analysis.
article type	research-article
publisher identifier	eas1257006
is part of this journal	EAS Publications Series

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