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
    Constraining the dark matter distribution in the centre of early-type barred galaxies
    The dynamics of a barred galaxy depends on the pattern speed of its bar. The only direct method for measuring the pattern speed of a bar is the Tremaine-Weinberg technique. This method is best suited to the analysis of the distribution and dynamics of the stellar component. Therefore it has been mostly used for early-type barred galaxies. Nearly
    Corsini, Enrico Maria et al.

    Advertised on:

    8
    2007
    Bibcode
    2007dyga.confE...4C
    Citations
    0
  • Refereed
    Chemical Properties of Star-Forming Dwarf Galaxies
    Recent studies of the near-infrared (NIR) properties of dwarf irregular galaxies (dIs) and blue compact dwarfs (BCDs) have provided improved estimates for the NIR luminosity of old stellar populations in these galaxies. These can be used to derive gas fractions, and thereby to evaluate how BCDs have evolved with respect to dIs. Oxygen abundances
    Vaduvescu, Ovidiu et al.

    Advertised on:

    8
    2007
    Bibcode
    2007AJ....134..604V
    Citations
    40
  • Non-refereed
    Brown dwarfs and star forming regions in the framework of the Spanish Virtual Observatory
    In this paper we describe three lines of work that are being developed in the framework of the Spanish Virtual Observatory.
    Solano, Enrique et al.

    Advertised on:

    8
    2007
    Bibcode
    2007HiA....14..597S
    Citations
    0
  • Non-refereed
    BH mass determination of low redshift quasars
    We present the analysis of the photometric and spectroscopic properties of a sample of 29 low redshift (z 0.6) QSOs for which both HST WFPC2 optical images and ultraviolet HST FOS spectra are available. For each object we measure the R band absolute magnitude of the host galaxy, the C IV (1550 Å) line width and the 1350 Å continuum luminosity
    Labita, M. et al.

    Advertised on:

    8
    2007
    Bibcode
    2007AIPC..924..858L
    Citations
    0