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
    The Initial-Final Mass Relationship of White Dwarfs in Common Proper Motion Pairs and Open Clusters
    The initial-to-final mass relationship is the connection between the mass of a white dwarf and the mass of its progenitor in the main sequence. This function is of paramount importance to aspects such as determining ages and distances of globular clusters, constraining the chemical evolution in galaxies, and also understanding the properties of the
    Catalán, S. et al.

    Advertised on:

    8
    2007
    Bibcode
    2007IAUS..240..380C
    Citations
    0
  • Non-refereed
    The edges of the stellar populations of early type spirals as probed by their radial brightness profiles
    Not Available
    Beckman, J. et al.

    Advertised on:

    8
    2007
    Bibcode
    2007IAUS..241..495B
    Citations
    0
  • Refereed
    The Discovery of a Companion to the Lowest Mass White Dwarf
    We report the detection of a radial velocity companion to SDSS J091709.55+463821.8, the lowest mass white dwarf currently known, with M~0.17 Msolar. The radial velocity of the white dwarf shows variations with a semi-amplitude of 148.8+/-6.9 km s-1 and a period of 7.5936+/-0.0024 hr, which implies a companion mass of M>=0.28 Msolar. The lack of
    Kilic, Mukremin et al.

    Advertised on:

    8
    2007
    Bibcode
    2007ApJ...664.1088K
    Citations
    34
  • Refereed
    The Color-Magnitude Distribution of Field Galaxies to z~3: The Evolution and Modeling of the Blue Sequence
    Using deep NIR VLT ISAAC and optical HST WFPC2 imaging in the HDF-S and MS 1054-03, we study the rest-frame UV-to-optical colors and magnitudes of galaxies to z~3. Unlike the present day, there is no evidence for a red sequence at z~3, but there does appear to be a well-defined CMR for blue galaxies at all redshifts, with more luminous galaxies
    Labbé, Ivo et al.

    Advertised on:

    8
    2007
    Bibcode
    2007ApJ...665..944L
    Citations
    42
  • Non-refereed
    The Cepheids Variable Stars Population in the Local Group Dwarf Irregular Galaxy Pegasus
    Not Available
    Meschin, I. et al.

    Advertised on:

    8
    2007
    Bibcode
    2007IAUS..241..365M
    Citations
    0
  • Non-refereed
    The ACS LCID project: overview and first results
    The star formation history (SFH) of Local Group galaxies is a powerful tool for studying their evolution, including chemical enrichment histories and stellar population gradients, which in turn may shed light on the role of reionization or Supernovae feedback in galaxy formation and evolution. In particular, isolated dwarfs are ideal laboratories
    Gallart, Carme et al.

    Advertised on:

    8
    2007
    Bibcode
    2007IAUS..241..290G
    Citations
    11