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

  • Supernova 1992bb in IRAS 21156-0747
    IAUC 5634 available at Central Bureau for Astronomical Telegrams. IAUC 5634 available at Central Bureau for Astronomical Telegrams.
    della Valle, M. et al.

    Fecha de publicación:

    10
    1992
    Número de citas
    5
  • Supernovae 1990U, 1990X, 1990aa
    IAUC 5129 available at Central Bureau for Astronomical Telegrams. IAUC 5129 available at Central Bureau for Astronomical Telegrams.
    Lopez, R. et al.

    Fecha de publicación:

    10
    1990
    Número de citas
    1
  • Supersonic Downflows in the Photosphere Discovered in Sunspot Moat Regions
    This paper reports on our new findings from the International Time Program observations at the Canaries islands, Spain, in July 2005. We have found small-scale photospheric events with extremely red-shifted Stokes V signals in sunspot moat regions. A preliminary estimate of the physical conditions for an observed Stokes V profile indicates the
    Shimizu, T. et al.

    Fecha de publicación:

    10
    2007
    Número de citas
    8
  • Supersonic Line Broadening and the Gas Dynamical Evolution of Giant HII Regions
    We have analyzed high spatial and spectral resolution Hα emission-line TAURUS data on two nearby giant H II regions, NGC 604 and NGC 588. Previous work shows that while NGC 604 is a relatively young system whose emission line kinematics is due to a combination of gravity and stellar wind-blown shells, NGC 588 seems more evolved, with its ionized
    Munoz-Tunon, C. et al.

    Fecha de publicación:

    10
    1996
    Número de citas
    55
  • Supersonic Motions in Giant H II Regions: Handling 3D Data with Matador
    Bidimensional spectroscopy with good spatial and spectral resolution, sampling a particular emission line over the whole emitting area, is shown here to be the most suitable observational technique for understanding the kinematics of giant extragalactic H II regions (GEHRs). The TAURUS II Fabry-Perot spectrograph is an excellent instrument for this
    Munoz-Tunon, C. et al.

    Fecha de publicación:

    10
    1995
    Número de citas
    18
  • Surface Brightness and Stellar Populations at the Outer Edge of the Large Magellanic Cloud: No Stellar Halo Yet
    We present a high-quality color-magnitude diagram (CMD) for a 36'×36' field located 8° (~=7 kpc) from the Large Magellanic Cloud (LMC) center, as well as a precise determination of the LMC surface brightness derived from the resolved stellar population out to this large galactocentric radius. This deep CMD shows for the first time the detailed age
    Gallart, Carme et al.

    Fecha de publicación:

    10
    2004
    Número de citas
    42