Abundance anomalies in hot horizontal branch stars of the galactic globular cluster NGC 1904

D. Fabbian*, A. Recio-Blanco, R. G. Gratton, G. Piotto

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    39 Citations (Scopus)

    Abstract

    We present abundance measurements, based on high-resolution optical spectroscopic data obtained with the Ultraviolet and Visual Echelle Spectrograph mounted on Kueyen (Very Large Telescope UT2), for ten stars in the extended blue horizontal branch of the Galactic globular cluster NGC 1904 (M79). In agreement with previous findings for other clusters, we obtain normal abundances for stars cooler than Teff ∼11000 K, and largely anomalous abundances for hotter stars: large He depletions, and overabundances of Fe, Ti, Cr, P and Mn. The abundances of Mg, Si and Ca are roughly normal, in the hot stars as well as in the cooler ones. This abundance pattern can be attributed to the onset of diffusion and to radiation pressure in the stable atmospheres of hot horizontal branch stars.

    Original languageEnglish
    Pages (from-to)235-245
    Number of pages11
    JournalAstronomy and Astrophysics
    Volume434
    Issue number1
    DOIs
    Publication statusPublished - Apr 2005

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