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/

  • Magnetic field emergence in mesogranular-sized exploding granules observed with sunrise/IMaX data
    We report on magnetic field emergences covering significant areas of exploding granules. The balloon-borne mission Sunrise provided high spatial and temporal resolution images of the solar photosphere. Continuum images, longitudinal and transverse magnetic field maps and Dopplergrams obtained by IMaX onboard Sunrise are analyzed by local
    Palacios, J. et al.

    Advertised on:

    1
    2012
    Citations
    27
  • Luminosity and mass functions of the three main sequences of the globular cluster NGC 2808
    High-precision HST photometry has revealed that the globular cluster (GC) NGC 2808 hosts a triple main sequence (MS) corresponding to three stellar populations with different helium abundances. We carried out photometry on ACS/WFC HST images of NGC 2808 with the main purpose of measuring the luminosity function (LF) of stars in the three different
    Milone, A. P. et al.

    Advertised on:

    1
    2012
    Citations
    71
  • Local Tadpole Galaxies
    Tadpole galaxies have a giant star-forming region at the end of an elongated intensity distribution. The origin of this asymmetric structure is not known, although suggestions range from ram pressure to mergers. We use SDSS data to determine the ages, masses, surface densities, and star formation rates of the heads and tails in 13 local tadpoles
    Elmegreen, Debra M. et al.

    Advertised on:

    1
    2012
    Citations
    0
  • LA GRAN NUBE DE MAGALLANES: HISTORIA DE LA FORMACION ESTELAR, ESTRUCTURA Y EVOLUCION
    INGRID PATRICIA MESCHIN

    Advertised on:

    1
    2012
  • LA GRAN NUBE DE MAGALLANES: HISTORIA DE LA FORMACIÓN ESTELAR, ESTRUCTURA Y EVOLUCIÓN
    El proceso de formación y evolución de las galaxias está determinado por dos conjuntos de mecanismos paralelos: (i) el ensamblado de la masa y sus interacciones con otros sistemas, que determinan su tipo morfológico y su evolución dinámica, que a su vez, induce formación estelar, y (ii) la formación, evolución y muerte estelar, que hace evolucionar
    Ingrid Patricia Meschin

    Advertised on:

    1
    2012