The giants stars HE 0107-5240 and HE 0557-4840 and new searches for metal-poor stars

Norbert Christlieb*, Andreas J. Korn, Kjell Eriksson, Michael S. Bessell, John E. Norris, Stefan C. Keller, Yongheng Zhao, Haotong Zhang, Timothy C. Beers

*Corresponding author for this work

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    Abstract

    We report on a new determination of the iron abundance of HE 0107-5240, based on the detection of two Fe II lines in an UV spectrum of the star, which yields [Fe/H]=-5.7. Another interesting metal-poor star recently discovered with Hamburg/ESO Survey (HES) is HE 0557-4840. With [Fe/H]=-4.8, it is the first star located in the "gap" in the metallicity distribution function of the galactic halo, in metallicity between the two stars known at [Fe/H]>-4.0. HE 0557-4840 is carbon-enhanced (i.e., [C/Fe]=+1.7). The abundance ratios of the heavier elements are similar to those seen in the majority of the metal-poor stars at [Fe/H]>-4.0. We also describe two upcoming wide-angle surveys which will be used for searches for metal-poor stars: The Southern Sky Survey (SSS), and a stellar survey to be conducted with the Chinese LAMOST telescope. These efforts are expected to increase the number of known extremely metal-poor stars, including stars below [Fe/H]=-5.0, by about two orders of magnitude.

    Original languageEnglish
    Title of host publicationFirst Stars III
    Pages109-112
    Number of pages4
    DOIs
    Publication statusPublished - 2008
    EventFirst Stars III - Santa Fe, NM, United States
    Duration: 15 Jul 200720 Jul 2007

    Publication series

    NameAIP Conference Proceedings
    Volume990
    ISSN (Print)0094-243X
    ISSN (Electronic)1551-7616

    Conference

    ConferenceFirst Stars III
    Country/TerritoryUnited States
    CitySanta Fe, NM
    Period15/07/0720/07/07

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