Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Sin árbitro
    Supernova 1990E in NGC 1035
    IAUC 5131 available at Central Bureau for Astronomical Telegrams. IAUC 5131 available at Central Bureau for Astronomical Telegrams.
    Lopez, R. et al.

    Fecha de publicación:

    11
    1990
    Bibcode
    1990IAUC.5131....2L
    Número de citas
    1
  • Sin árbitro
    Supernova 2004ao in UGC 10862
    IAUC 8430 available at Central Bureau for Astronomical Telegrams.
    Gomez, G. et al.

    Fecha de publicación:

    11
    2004
    Bibcode
    2004IAUC.8430....2G
    Número de citas
    4
  • Con árbitro
    Supernovae and Their Expanding Blast Waves during the Early Evolution of Galactic Globular Clusters
    Our arguments deal with the early evolution of Galactic globular clusters and show why only a few of the supernovae (SNe) products were retained within globular clusters and only in the most massive cases (M ≥ 106 M⊙), while less massive clusters were not contaminated at all by SNe. Here, we show that SN blast waves evolving in a steep density
    Tenorio-Tagle, G. et al.

    Fecha de publicación:

    11
    2015
    Bibcode
    2015ApJ...814L...8T
    Número de citas
    23
  • Con árbitro
    Supersonic Magnetic Upflows in Granular Cells Observed with SUNRISE/IMAX
    Using the IMaX instrument on board the SUNRISE stratospheric balloon telescope, we have detected extremely shifted polarization signals around the Fe I 5250.217 Å spectral line within granules in the solar photosphere. We interpret the velocities associated with these events as corresponding to supersonic and magnetic upflows. In addition, they are
    Borrero, J. M. et al.

    Fecha de publicación:

    11
    2010
    Bibcode
    2010ApJ...723L.144B
    Número de citas
    48
  • Con árbitro
    Suppression of cooling by strong magnetic fields in white dwarf stars
    Isolated cool white dwarf stars more often have strong magnetic fields than young, hotter white dwarfs, which has been a puzzle because magnetic fields are expected to decay with time but a cool surface suggests that the star is old. In addition, some white dwarfs with strong fields vary in brightness as they rotate, which has been variously
    Valyavin, G. et al.

    Fecha de publicación:

    11
    2014
    Bibcode
    2014Natur.515...88V
    Número de citas
    53