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

  • Three-dimensional structure of a sunspot light bridge
    Context. Active regions are the most prominent manifestations of solar magnetic fields; their generation and dissipation are fundamental problems in solar physics. Light bridges are commonly present during sunspot decay, but a comprehensive picture of their role in the removal of the photospheric magnetic field is still lacking. Aims: We study the
    Felipe, T. et al.

    Fecha de publicación:

    11
    2016
    Número de citas
    44
  • Toward an Internally Consistent Astronomical Distance Scale
    Accurate astronomical distance determination is crucial for all fields in astrophysics, from Galactic to cosmological scales. Despite, or perhaps because of, significant efforts to determine accurate distances, using a wide range of methods, tracers, and techniques, an internally consistent astronomical distance framework has not yet been
    de Grijs, R. et al.

    Fecha de publicación:

    11
    2017
    Número de citas
    26
  • Towards a dynamical mass of the ultraluminous X-ray source NGC 5408 X-1
    We obtained multi-epoch Very Large Telescope optical spectroscopic data in 2011 and 2012 on the ultraluminous X-ray source NGC 5408 X-1. We confirm that the He II λ4686 line has a broad component with an average full width at half-maximum of v = 780 ± 64 km s-1 with a variation of ˜13 per cent during observations spanning over four years, and is
    Grisé, F. et al.

    Fecha de publicación:

    11
    2013
    Número de citas
    19
  • Tracing Chemical Evolution over the Extent of the Milky Way's Disk with APOGEE Red Clump Stars
    We employ the first two years of data from the near-infrared, high-resolution SDSS-III/APOGEE spectroscopic survey to investigate the distribution of metallicity and α-element abundances of stars over a large part of the Milky Way disk. Using a sample of ≈10, 000 kinematically unbiased red-clump stars with ~5% distance accuracy as tracers, the [α
    Nidever, D. L. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    195
  • Tracing the coronal emission in Circinus with VLT/NACO
    In this short letter we present our new work on the coronal emission in a sample of AGN. We used the adaptive optics system NACO on the VLT to obtain high angular resolution images (˜0.15') of the coronal emission in the vicinity of the central engine.
    Marco, Olivier et al.

    Fecha de publicación:

    11
    2004
    Número de citas
    0
  • Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA
    Our current knowledge of star formation and accretion luminosity at high redshift (z > 3-4), as well as the possible connections between them, relies mostly on observations in the rest-frame ultraviolet, which are strongly affected by dust obscuration. Due to the lack of sensitivity of past and current infrared instrumentation, so far it has not
    Gruppioni, C. et al.

    Fecha de publicación:

    11
    2017
    Número de citas
    21