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/

  • Non-refereed
    Galaxy morphology in 5 medium redshift clusters (Ascaso+, 2009)
    Following the study presented in our previous paper, based on the Nordic Optical Telescope (NOT) sample, which consists of five clusters of galaxies within the redshift range 0.18
    Ascaso, B. et al.

    Advertised on:

    9
    2010
    Bibcode
    2010yCat..35061071A
    Citations
    0
  • Refereed
    Galactic evolution of oxygen. OH lines in 3D hydrodynamical model atmospheres
    Context. Oxygen is the third most common element in the Universe. The measurement of oxygen lines in metal-poor unevolved stars, in particular near-UV OH lines, can provide invaluable information about the properties of the Early Galaxy. Aims: Near-UV OH lines constitute an important tool to derive oxygen abundances in metal-poor dwarf stars
    González Hernández, J. I. et al.

    Advertised on:

    9
    2010
    Bibcode
    2010A&A...519A..46G
    Citations
    35
  • Thesis
    EVOLUCIÓN QUÍMICA DE GALAXIAS UTILIZANDO EL SDSS
    Premio Extraordinario de Doctorado 2010
    MARITZA ARLENE LARA LÓPEZ

    Advertised on:

    9
    2010
  • Refereed
    Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry
    Aims: Using the CoRoT space based photometry of the O-type binary HD 46149, stellar atmospheric effects related to rotation can be separated from pulsations, because they leave distinct signatures in the light curve. This offers the possibility of characterising and exploiting any pulsations seismologically. Methods: Combining high-quality space
    Degroote, P. et al.

    Advertised on:

    9
    2010
    Bibcode
    2010A&A...519A..38D
    Citations
    59
  • Refereed
    Decreased Frequency of Strong Bars in S0 Galaxies: Evidence for Secular Evolution?
    Using data from the Near-Infrared S0 Survey of nearby, early-type galaxies, we examine the distribution of bar strengths in S0 galaxies as compared to S0/a and Sa galaxies, and as compared to previously published bar strength data for Ohio State University Bright Spiral Galaxy Survey spiral galaxies. Bar strengths based on the gravitational torque
    Buta, R. et al.

    Advertised on:

    9
    2010
    Bibcode
    2010ApJ...721..259B
    Citations
    48