Chemical abundances in 31 stars with planet (Gonzalez+, 2007)

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We focus on the 31 SWPs examined in Laws et al. (2003AJ....125.2664L) (here, we are now including HD 202206 amongst the SWP sample for comparison purposes in this paper). We measured equivalent widths (EWs) for atomic lines of C, N, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, Cr, Ni, Zn and Eu.
(6 data files).

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