Abundances of BHB stars in NGC 1904 (Fabbian+, 2005)

Physics

Scientific paper

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Clusters: Globular, Equivalent Widths

Scientific paper

The abundance measurements are based on high-resolution optical spectroscopical data, obtained during 2 observing runs with the Ultraviolet and Visual Echelle Spectrograph mounted on Kueyen (Very Large Telescope UT2). Ten target stars in the extended blue horizontal branch of the Galactic globular cluster NGC 1904 (M79) have been analysed.
(2 data files).

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