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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  • Star Formation in the Spiral Arms of NGC 4321. II. H i Distribution and Kinematics
    We present H I 21 cm observations of the grand design spiral galaxy NGC 4321, as obtained with the VLA. From our original data, we have obtained data cubes with resolutions ranging from 13" to 45". The H I is observed to break up into small condensations at high resolution. These condensations, with typical masses of 3.3±0.7 × 107 Msun, are not
    Knapen, J. H. et al.

    Fecha de publicación:

    10
    1993
    Número de citas
    74
  • Star-gas decoupling and a non-rotating stellar core in He 2-10. Integral field spectroscopy with FLAMES/ARGUS
    Aims:We study the two-dimensional distribution and kinematics of the stellar and gaseous components in the centre of the blue compact dwarf galaxy He 2-10. The aim is to compare the kinematics of gas and stars in order to determine whether they are consistent with one another, or if stars and gas can be decoupled due to gravitational perturbations
    Marquart, T. et al.

    Fecha de publicación:

    10
    2007
    Número de citas
    18
  • STARE operations experience and its data quality control
    The STARE instrument was the first to detect the transits of an extrasolar planet in 1999. To date it has performed one of the longest running searches for transits, being in nearly continous operations since July 2001 at Teide Observatory, Tenerife. We describe the instrumental setup and the scheme that is used for data acquisition, handling and
    Alonso, R. et al.

    Fecha de publicación:

    10
    2004
    Número de citas
    13
  • Stars and brown dwarfs in the σ Orionis cluster. III. OSIRIS/GTC low-resolution spectroscopy of variable sources
    Context. Although many studies have been performed so far, there are still dozens of low-mass stars and brown dwarfs in the young σ Orionis open cluster without detailed spectroscopic characterisation. Aims: We look for unknown strong accretors and disc hosts that were undetected in previous surveys. Methods: We collected low-resolution
    Caballero, J. A. et al.

    Fecha de publicación:

    10
    2012
    Número de citas
    9
  • Statistical properties of magnetic fields in intranetwork
    We report a study of the quiet sun's magnetic field based on high-resolution infrared spectropolarimetric observations (TIP/VTT). We find that in almost 50% of the pixels Stokes V and in 15% the Stokes Q and/or U profiles have a signal above 10-3. The statistical properties of the mainly intranetwork field sampled by these observations are
    Khomenko, E. V. et al.

    Fecha de publicación:

    10
    2002
    Número de citas
    0
  • Statistical turbulence vertical profiles at the Roque de los Muchachos Observatory and Teide Observatory
    The characterization of the vertical turbulence distribution on an astronomical site should be based on statistical behaviour, as it is required for other parameters in site testing. We present the statistical results of the optical-turbulence profiles at the Roque de los Muchachos and Teide observatories at the Canary Islands (Spain). The data
    García-Lorenzo, B. et al.

    Fecha de publicación:

    10
    2007
    Número de citas
    0