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/

  • Refereed
    The Large Magellanic Cloud as a laboratory for hot bottom burning in massive asymptotic giant branch stars
    We use Spitzer observations of the rich population of asymptotic giant branch (AGB) stars in the Large Magellanic Cloud (LMC) to test models describing the internal structure and nucleosynthesis of the most massive of these stars, i.e. those with initial mass above ˜4 M⊙. To this aim, we compare Spitzer observations of LMC stars with the
    Ventura, P. et al.

    Advertised on:

    7
    2015
    Bibcode
    2015MNRAS.450.3181V
    Citations
    44
  • Refereed
    The initial mass function of a massive relic galaxy
    Massive relic galaxies formed the bulk of their stellar component before z ˜ 2 and have remained unaltered since then. Therefore, they represent a unique opportunity to study in great detail the frozen stellar population properties of those galaxies that populated the primitive Universe. We have combined optical to near-infrared line-strength
    Martín-Navarro, I. et al.

    Advertised on:

    7
    2015
    Bibcode
    2015MNRAS.451.5600M
    Citations
    0
  • Refereed
    The initial mass function of a massive relic galaxy
    Massive relic galaxies formed the bulk of their stellar component before z ˜ 2 and have remained unaltered since then. Therefore, they represent a unique opportunity to study in great detail the frozen stellar population properties of those galaxies that populated the primitive Universe. We have combined optical to near-infrared line-strength
    Martín-Navarro, I. et al.

    Advertised on:

    7
    2015
    Bibcode
    2015MNRAS.451.1081M
    Citations
    79
  • Refereed
    The impact of surface dynamo magnetic fields on the solar iron abundance
    Most chemical abundance determinations ignore that the solar photosphere is significantly magnetized by the ubiquitous presence of a small-scale magnetic field. A recent investigation has suggested that there should be a significant impact on the derived iron abundance, owing to the magnetically induced changes on the photospheric temperature and
    Trujillo Bueno, J. et al.

    Advertised on:

    7
    2015
    Bibcode
    2015A&A...579A.112S
    Citations
    15
  • Refereed
    The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters - IV. Helium content and relative age of multiple stellar populations within NGC 6352
    In this paper, we combine Wide Field Camera3/UVIS F275W, F336W, and F438W data from the `UV Legacy Survey of Galactic Globular Clusters: Shedding Light on Their Populations and Formation' (GO 13297) Hubble Space Telescope Treasury programme with F606W, F625W, F658N, and F814W Advanced Camera for Surveys archive data for a multiwavelength study of
    Nardiello, D. et al.

    Advertised on:

    7
    2015
    Bibcode
    2015MNRAS.451.4831N
    Citations
    0
  • Refereed
    The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters - IV. Helium content and relative age of multiple stellar populations within NGC 6352
    In this paper, we combine Wide Field Camera3/UVIS F275W, F336W, and F438W data from the `UV Legacy Survey of Galactic Globular Clusters: Shedding Light on Their Populations and Formation' (GO 13297) Hubble Space Telescope Treasury programme with F606W, F625W, F658N, and F814W Advanced Camera for Surveys archive data for a multiwavelength study of
    Nardiello, D. et al.

    Advertised on:

    7
    2015
    Bibcode
    2015MNRAS.451..312N
    Citations
    55