Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S268(5), p. 291-299, 2009
DOI: 10.1017/s1743921310004266
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Light elements in stars with exoplanets
Journal article published in 2009 by
N. C. Santos,
E. Delgado Mena,
G. Israelian,
J. I. González-Hernández 
,
M. C. Gálvez-Ortiz,
M. Mayor,
S. Udry,
R. Rebolo ,
S. Sousa ,
S. Randich
,
M. C. Gálvez-Ortiz,
M. Mayor,
S. Udry,
R. Rebolo ,
S. Sousa ,
S. Randich
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
AbstractIt 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.
