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..

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  • 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
    Número de citas
    23
  • 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
    Número de citas
    48
  • 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
    Número de citas
    53
  • Surface photometry and spectral analysis of Mk50 - A Seyfert 1 nucleus in an early type galaxy
    Markarian 50 is analyzed using V and I CCD frames and IPCS and CCD spectra, obtained in June 1985, covering the range 3200-10,000 A. It is inferred from the surface brightness profiles derived from the images that this is an early-type, elliptical, or S0 galaxy, which is supported by the spectral analysis of the stellar population. After
    Pastoriza, M. G. et al.

    Fecha de publicación:

    11
    1991
    Número de citas
    1
  • Surface Waves in Solar Granulation Observed with SUNRISE
    Solar oscillations are expected to be excited by turbulent flows in the intergranular lanes near the solar surface. Time series recorded by the IMaX instrument on board the SUNRISE observatory reveal solar oscillations at high spatial resolution, which allow the study of the properties of oscillations with short wavelengths. We analyze two time
    Roth, M. et al.

    Fecha de publicación:

    11
    2010
    Número de citas
    26
  • SWEET-Cat updated. New homogenous spectroscopic parameters
    Context. Exoplanets have now been proven to be very common. The number of its detections continues to grow following the development of better instruments and missions. One key step for the understanding of these worlds is their characterization, which mostly depend on their host stars. Aims: We perform a significant update of the Stars With
    Sousa, S. G. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    69