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    Chapter and Conference Paper

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    Many talks in this conference have shown the power of high resolution spectroscopy, coupled to high precision. A new spectrograph, fed by an Extremely Large Telescope, will have such a huge collecting power th...

    Luca Pasquini, G. Avila, B. Délabre, H. Dekker in Precision Spectroscopy in Astrophysics (2008)

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    Chapter and Conference Paper

    Abundances in Damped Lyα Galaxies

    Damped Lyα galaxies provide a sample of young galaxies where chemical abundances can be derived throughout the whole universe with an accuracy comparable to that for the local universe. Despite a large spread ...

    P. Molaro in Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites (2006)

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    Chapter and Conference Paper

    Evidence of Mixing in Extremely Metal-Poor Giants

    Thirty five extremely metal-poor (EMP) giants (22 of them with a metallicity [Fe/H] ≤ -3.0) have been observed with UVES at the VLT. In these stars the abundance of lithium carbon and nitrogen and also the 12C/13

    M. Spite, R. Cayrel, F. Spite, V. Hill in Chemical Abundances and Mixing in Stars in… (2006)

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    Chapter and Conference Paper

    Abundance of Heavy Elements in Extremely Metal-Poor Stars

    In the framework of the VLT Large program “First Stars” (165.N-0276(A)), we have measured the abundance of 13 heavy elements using high quality UVES spectra. In this paper, we report on the abundance of Sr and...

    P. François1, R. Cayrel, E. Depagne in Chemical Abundances and Mixing in Stars in… (2006)

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    Chapter and Conference Paper

    Abundances in Sagittarius Stars

    The Sagittarius dwarf spheroidal is a very complex galaxy, which has undergone prolonged star formation. From the very first high resolution chemical analysis of Sgr stars, conducted using spectra obtained dur...

    P. Bonifacio, S. Zaggia, L. Sbordone in Chemical Abundances and Mixing in Stars in… (2006)