Chemical abundances in Leo I and II dSph (Bosler+, 2007)

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Galaxies: Nearby, Abundances, Equivalent Widths

Scientific paper

The photometry and astrometry for Leo I and II were obtained as part of a larger program to provide homogeneous photometry for star clusters and nearby resolved galaxies (e.g. Stetson, Hesser & Smecker-Hane 1998, Cat. ; Stetson 2000PASP..112..925S). The present photometry is based upon a large database of CCD images acquired by ourselves and collaborators, images obtained from the archives of the Canada-France-Hawaii Telescope and the Isaac Newton Group and images privately donated by other astronomers.
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