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Lithium abundances in exoplanet host stars as test of planetary formation scenarii

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 2005Embargo end date: 01 Jan 2005Publisher:EDP SciencesJournal:EAS Publications Series, volume 17, pages 297-300 (issn: 1633-4760, eissn: 1638-1963, Copyright policy )
Authors: Castro, M.; Richard, O.; Vauclair, S.;

doi: 10.1051/eas:2005126 , 10.1017/s1743921305005284 , 10.48550/arxiv.astro-ph/0510615

arXiv: http://arxiv.org/abs/astro-ph/0510615

Lithium abundances in exoplanet host stars as test of planetary formation scenarii

Abstract

Following the observations of Israelian et al. 2004, we compare different evolutionary models in order to study the lithium destruction processes and the planetary formation scenarii.

4 pages, 5 figures, proceeding of the meeting "Element Stratification in stars : 40 years of atomic diffusion", Mons 6-11 Juin 2005

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Astrophysics (astro-ph), FOS: Physical sciences, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Astrophysics

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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