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

  • A Statistical Inference Method for Interpreting the CLASP Observations
    On 2015 September 3, the Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) successfully measured the linear polarization produced by scattering processes in the hydrogen Lyα line of the solar disk radiation, revealing conspicuous spatial variations in the Q/I and U/I signals. Via the Hanle effect, the line-center Q/I and U/I amplitudes encode
    Štěpán, J. et al.

    Fecha de publicación:

    9
    2018
    Número de citas
    3
  • A statistical study of the geometrical Wilson effect
    An analysis has been carried out of the center-to-limb variation of the apparent sizes of the umbra, penumbra, and whole spot. It has revealed that the umbral size decreases with height. This result is interpreted in terms of the penumbral geometrical height scale. A value of 230 km, which is larger than that of the photosphere or the umbra
    Collados, M. et al.

    Fecha de publicación:

    9
    1987
    Número de citas
    12
  • A Stellar Model-fitting Pipeline for Solar-like Oscillations
    Over the past two decades, helioseismology has revolutionized our understanding of the interior structure and dynamics of the Sun. Asteroseismology will soon place this knowledge into a broader context by providing structural data for hundreds of Sun-like stars. Solar-like oscillations have already been detected from the ground in several stars
    Metcalfe, T. S. et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    1
  • A study of the neglected Galactic H ii region NGC 2579 and its companion ESO 370-9
    Context: The Galactic H ii region NGC 2579 has stayed undeservedly unexplored due to identification problems which persisted until recently. Both NGC 2579 and its companion ESO 370-9 have been misclassified as planetary or reflection nebula, confused with each other and with other objects. Due to its high surface brightness, high excitation
    Copetti, M. V. F. et al.

    Fecha de publicación:

    9
    2007
    Número de citas
    17
  • A survey of faint, near-infrared sources towards the centre of the Galaxy
    The authors present the results of a survey made at 1.65 μm (H) and 2.2 μm (K) in 15 small areas on the galactic equator between l = 0° and l = 10°. 775 distinct objects were counted in a total area of 0.17 deg2 to limiting magnitudes H = 10.5 and K = 9.5 (equivalent to detecting M giants at 6 - 7 kpc). Source confusion was the limiting factor in
    Jones, A. W. et al.

    Fecha de publicación:

    9
    1984
    Número de citas
    7
  • A Technique for Separating the Gravitational Torques of Bars and Spirals in Disk Galaxies
    We describe a Fourier-based method of separating bars from spirals in near-infrared images. The method takes advantage of the fact that a bar is typically a feature with a relatively fixed position angle and uses the simple assumption that the relative Fourier amplitudes due to the bar decline with radius past a maximum in the same or a similar
    Buta, R. et al.

    Fecha de publicación:

    9
    2003
    Número de citas
    53