Publication type: Non-refereed

  • Publication
    Overview of the status of the European Solar Telescope
    The European Solar Telescope (EST) aims to become the most ambitious ground-based solar telescope in Europe. Its roots lie in the knowledge and expertise gained...
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    Oxygen abundance from strong-line methods at extremely low metallicities
    The determination of oxygen abundance in nebulae requires measuring a significant number of emission lines distributed along a wide spectral range. The required...
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    Oxygen abundance in M101 HII regions (Cedres+, 2004)
    We present the oxygen abundance determination for 90 HII regions in the inner parts of the grand design galaxy M101. The abundances were derived employing the P...
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    Oxygen abundance profiles with MUSE: Radial gradients and widespread deviations
    This study has been published in Sánchez-Menguiano et al. (2018). We encourage the reader to that article for more details on the study and the results.
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    Oxygen abundances derived from UV OH and O I IR lines in very metal-poor stars
    Oxygen abundances have been derived in a sample of very metal-poor stars using the O I triplet at λλ7771-5 Å and OH lines in the near UV. A detailed NLTE...
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    Oxygen Abundances derived from UV OH Lines
    The reliability of oxygen abundances derived from OH UV lines in metal-poor dwarf stars is discussed in the light of the stellar parameters adopted and the...
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    Oxygen abundances in Li-depleted F-type stars
    Not Available
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    Oxygen abundances in nearby stars (Ramirez+, 2007)
    We provide in Table 4 basic (HIP and HD numbers, V magnitude and parallax) and kinematic (radial velocities and heliocentric space velocity) data for our sample...
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    Oxygen abundances in old disc and halo stars of the Galaxy
    Intermediate resolution CCD spectra of the oxygen triplet at 7770 A have been analyzed to determine oxygen abundances in a sample of metal-deficient stars with...