June 3, 2013 (v1)
Conference paper
Royer et al. (2007) studied a sample of A0-A1 stars that did not contain any previously known binary or chemically peculiar (CP) star. They showed that the distribution of the equatorial rotational velocities of the sample is bimodal. We report here the preliminary results of the abundance analysis of 47 of those ``normal'' A0-A1 main-sequence...
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