Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Two new confirmed massive relic galaxies: red nuggets in the present-day Universe
    We confirm two new local massive relic galaxies, i.e. untouched survivors of the early Universe massive population: Mrk 1216 and PGC 032873. Both show early and peaked formation events within very short time-scales ( 2 massive population, setting them apart from the typical z ∼ 0 massive early-type galaxies. We find that there seems to exist a
    Ferré-Mateu, Anna et al.

    Fecha de publicación:

    5
    2017
    Número de citas
    99
  • The VLT-FLAMES Tarantula Survey. XXVI. Properties of the O-dwarf population in 30 Doradus
    Context. The VLT-FLAMES Tarantula Survey has observed hundreds of O-type stars in the 30 Doradus region of the Large Magellanic Cloud (LMC). Aims: We study the properties of a statistically significant sample of O-type dwarfs in the same star-forming region and test the latest atmospheric and evolutionary models of the early main-sequence phase of
    Sabín-Sanjulián, C. et al.

    Fecha de publicación:

    5
    2017
    Número de citas
    54
  • The imprints of bars on the vertical stellar population gradients of galactic bulges
    This is the second paper of a series aimed to study the stellar kinematics and population properties of bulges in highly inclined barred galaxies. In this work, we carry out a detailed analysis of the stellar age, metallicity and [Mg/Fe] of 28 highly inclined (i > 65°) disc galaxies, from S0 to S(B)c, observed with the SAURON integral-field
    Molaeinezhad, A. et al.

    Fecha de publicación:

    5
    2017
    Número de citas
    10
  • The GAPS Programme with HARPS-N at TNG. XIII. The orbital obliquity of three close-in massive planets hosted by dwarf K-type stars: WASP-43, HAT-P-20 and Qatar-2
    Context. The orbital obliquity of planets with respect to the rotational axis of their host stars is a relevant parameter for the characterization of the global architecture of planetary systems and a key observational constraint to discriminate between different scenarios proposed to explain the existence of close-in giant planets. Aims: In the
    Esposito, M. et al.

    Fecha de publicación:

    5
    2017
    Número de citas
    54
  • The effect of environment on the structure of disc galaxies
    We study the influence of environment on the structure of disc galaxies, using imfit to measure the g- and r-band structural parameters of the surface-brightness profiles for ∼700 low-redshift (z 0.063) cluster and field disc galaxies with intermediate stellar mass (0.8 × 1010 M⊙ M⋆ 4 × 1010 M⊙) from the Sloan Digital Sky Survey, DR7. Based on
    Pranger, Florian et al.

    Fecha de publicación:

    5
    2017
    Número de citas
    20
  • The Correlation between Mixing Length and Metallicity on the Giant Branch: Implications for Ages in the Gaia Era
    In the updated APOGEE-Kepler catalog, we have asteroseismic and spectroscopic data for over 3000 first ascent red giants. Given the size and accuracy of this sample, these data offer an unprecedented test of the accuracy of stellar models on the post-main-sequence. When we compare these data to theoretical predictions, we find a metallicity
    Tayar, Jamie et al.

    Fecha de publicación:

    5
    2017
    Número de citas
    108