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/

  • Stellar distribution in the Galactic disc from NIR color-magnitude diagrams
    We analyze the stellar distribution in the Galactic disc via NIR color-magnitude diagrams (CMDs). Extinction measurements in the K band are also extracted from the diagrams both for supporting stellar counts predictions of the Besançon and "SKY" models and for comparing with a three dimensional model of the Galactic extinction. The method is based
    Cabrera-Lavers, A. et al.

    Advertised on:

    12
    2004
    Citations
    0
  • Stellar Kinematics and Chemical Abundances at the Thick-Disk/Halo Interface
    The old stellar populations of the Milky Way carry the signature of their formation environment and dynamical history in their kinematics and chemical abundances. In particular, the dynamically hot thick disk and halo contain the oldest stars in the Galaxy, and are remnants of its more chaotic past. We present a study of the high-latitude thick
    Rockosi, C. M. et al.

    Advertised on:

    12
    2004
    Citations
    0
  • Stellar Kinematics and Structural Properties of Virgo Cluster Dwarf Early-type Galaxies from the SMAKCED Project. II. The Survey and a Systematic Analysis of Kinematic Anomalies and Asymmetries
    We present spatially resolved kinematics and global stellar populations and mass-to-light ratios for a sample of 39 dwarf early-type (dE) galaxies in the Virgo cluster studied as part of the SMAKCED stellar absorption-line spectroscopy and imaging survey. This sample is representative of the early-type population in the Virgo cluster in the
    Toloba, E. et al.

    Advertised on:

    12
    2014
    Citations
    60
  • Stellar masses of star-forming galaxies at 0.3 < z < 1.2 in the GOYA survey
    Starforming galaxies with compact morphology and high optical luminosity (LBCGs) are very common at redshitfs z = 0.4 - 1.2. Those galaxies are believed to have evolved more than other galaxy class during the last ~ 8 Gyr, and are a mayor contributor to the global star formation rate density of the universe at z ~ 1. A robust way to gauge their
    Cristóbal-Hornillos, D. et al.

    Advertised on:

    12
    2005
    Citations
    1
  • Stellar models for a wide range of initial chemical compositions until helium burning. II. From X=0.63 to X=0.80, for Z=0.01.
    Three new grids of stellar evolutionary models with Z=0.01 are presented for the following values of initial hydrogen content X_i_=0.80, 0.73 and 0.63. The latest set of radiative opacities with spin-orbit coupling provided by the Lawrence Livermore group are used. For the lower temperatures the results by Alexander were considered. The models were
    Gimenez, A. et al.

    Advertised on:

    12
    1995
    Citations
    43
  • Stellar p-mode oscillations signal in Procyon A from MOST data
    Recently, Matthews et al. (2004, Nature, 430, 51) claim a null detection of p-mode oscillations in Procyon A from 32 days of nearly continuous photometric satellite-based observations (MOST). They did not even find evidence in the Fourier amplitude spectrum of Procyon of the uniform frequency spacing signature that solar-like stars acoustic
    Régulo, C. et al.

    Advertised on:

    12
    2005
    Citations
    18