Abundances in stars with exoplanets

dc.creatorIsraelian, Garik
dc.date2003-10-14
dc.date.accessioned2026-07-07T02:10:24Z
dc.date.available2026-07-07T02:10:24Z
dc.descriptionExtensive spectroscopic studies of stars with and without planets have concluded that stars hosting planets are significantly more metal-rich than those without planets. More subtle trends of different chemical elements begin to appear as the number of detected extrasolar planetary systems continues to grow. I review our current knowledge concerning the observed abundance trends of various chemical elements in stars with exoplanets and their possible implications.
dc.description12 pages, 6 figures, to appear in IAU Symposium 219: Stars as Suns, Activity, Evolution and Planets, eds: A. K. Dupree and A. Benz
dc.identifierhttps://arxiv.org/abs/astro-ph/0310377
dc.identifierhttp://arxiv.org/abs/astro-ph/0310377
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6728
dc.subjectAstrophysics
dc.titleAbundances in stars with exoplanets
dc.typetext

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