Light elements in stars with exoplanets

Bibcode
2010IAUS..268..291S
DOI
10.1017/S1743921310004266
Santos, N. C.; Delgado-Mena, E.; Israelian, G.; González-Hernández, J. I.; Gálvez-Ortiz, M. C.; Mayor, M.; Udry, S.; Rebolo, R.; Sousa, S.; Randich, S.
Referencia bibliográfica

Light Elements in the Universe, Proceedings of the International Astronomical Union, IAU Symposium, Volume 268, p. 291-299

Advertised on:
4
2010
Número de autores
10
Número de autores del IAC
3
Número de citas
5
Número de citas referidas
4
Descripción
It is well known that stars orbited by giant planets have higher abundances of heavy elements when compared with average field dwarfs. A number of studies have also addressed the possibility that light element abundances are different in these stars. In this paper we will review the present status of these studies. The most significant trends will be discussed.
Tipo
Sin árbitro

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