NDLI: Lithium abundances in exoplanet host stars as a test for planetary formation scenarii

Content Provider	Scilit
Author	Castro, M. Richard, O. Vauclair, S.
Copyright Year	2005
Description	The observations of Israelian et al. (2004) show that, in an effective temperature range between 5600, 5850 K, the planet host stars present a significant lithium underabundance compared to the stars without planets. We have studied this phenomena in order to discriminate the different planetary formation scenarii.
Related Links	https://www.cambridge.org/core/services/aop-cambridge-core/content/view/62E5B22CAF43625EB645B1D125A89B87/S1743921305005284a.pdf/div-class-title-lithium-abundances-in-exoplanet-host-stars-as-a-test-for-planetary-formation-scenarii-div.pdf
Ending Page	86
Page Count	2
Starting Page	85
ISSN	17439213
e-ISSN	17439221
DOI	10.1017/s1743921305005284
Journal	Proceedings of the International Astronomical Union
Issue Number	S228
Volume Number	1
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2005-05-01
Access Restriction	Open
Subject Keyword	Proceedings of the International Astronomical Union Astronomy and Astrophysics Abundances Planetary Systems
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

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Lithium abundances in exoplanet host stars as a test for planetary formation scenarii