Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78
    Highly r-process-enhanced (RPE) stars are rare and usually metal poor ([Fe/H] < ‑1.0), and they mainly populate the Milky Way halo and dwarf galaxies. This study presents the discovery of a relatively bright (V = 12.72), highly RPE (r-II) star ([Eu/Fe] = +1.32, [Ba/Eu] = ‑0.95), LAMOST J020623.21+494127.9. This star was selected from the Large Sky
    Xie, Xiao-Jin et al.

    Advertised on:

    8
    2024
    Citations
    0
  • Mapping the oxygen abundance in Red Geysers and its relation with the gas kinematics using MEGACUBES
    Red Geysers are galaxies with low-star formation rates and galactic scale ionized outflows likely driven by low-luminosity active galactic nuclei (AGN). We investigated the impact of AGN winds on the oxygen abundance using integral field spectroscopic data from Mapping Nearby Galaxies for Red Geysers, control galaxies (quiescent galaxies without
    Ilha, Gabriele S. et al.

    Advertised on:

    8
    2024
    Citations
    0
  • First light simultaneous triple-channel optical observations of the OPTICAM system at the OAN-SPM
    OPTICAM is a triple-band optical system developed for the 2.1 m telescope of the National Astronomical Observatory in the Sierra de San Pedro Mártir (OAN-SPM). Partial engineering tests were conducted in 2019, with the complete system experiencing its first light in March 2022. The system incorporates two beam splitters, enabling simultaneous
    Castro, Angel et al.

    Advertised on:

    11
    2024
    Citations
    0
  • Euclid preparation. XLI. Galaxy power spectrum modelling in real space
    We investigate the accuracy of the perturbative galaxy bias expansion in view of the forthcoming analysis of the Euclid spectroscopic galaxy samples. We compare the performance of a Eulerian galaxy bias expansion using state-of-the-art prescriptions from the effective field theory of large-scale structure (EFTofLSS) with a hybrid approach based on
    Euclid Collaboration et al.

    Advertised on:

    7
    2024
    Citations
    6
  • OCCASO. V. Chemical-abundance trends with Galactocentric distance and age
    Context. Open clusters provide valuable information on stellar nucleosynthesis and the chemical evolution of the Galactic disk, as their age and distances can be measured more precisely with photometry than in the case of field stars. Aims: Our aim is to study the chemical distribution of the Galactic disk using open clusters by analyzing the
    Carbajo-Hijarrubia, J. et al.

    Advertised on:

    7
    2024
    Citations
    2
  • The IACOB project. XI. No increase in mass-loss rates over the bistability region
    The properties of blue supergiants are key for constraining the end of the main sequence (MS) of massive stars. Whether the observed drop in the relative number of fast-rotating stars below ≈21 kK is due to enhanced mass-loss rates at the location of the bistability jump, or the result of the end of the MS is still debated. Here, we combine newly
    de Burgos, A. et al.

    Advertised on:

    7
    2024
    Citations
    1