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

  • The Metallicity Planet Correlation In The Harps Volume Limited Sample
    To understand the formation and evolution of solar-type stars and planets in the solar neighborhood, we need to obtain their stellar parameters with high precision. We present a catalog of precise stellar parameters for the FGK stars in a volume limited sample followed by the HARPS spectrograph in the quest for extra solar planets. The
    Sousa, Sérgio et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    0
  • The Hanle Effect of the Hydrogen Lyα Line for Probing the Magnetism of the Solar Transition Region
    We present some theoretical predictions concerning the amplitude and magnetic sensitivity of the linear-polarization signals produced by scattering processes in the hydrogen Lyα line of the solar transition region. To this end, we have calculated the atomic-level polarization (population imbalances and quantum coherences) induced by anisotropic
    Trujillo-Bueno, J. et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    54
  • The excitation of solar-like oscillations in a δSct star by efficient envelope convection
    Delta Scuti (δSct) stars are opacity-driven pulsators with masses of 1.5-2.5Msolar, their pulsations resulting from the varying ionization of helium. In less massive stars such as the Sun, convection transports mass and energy through the outer 30per cent of the star and excites a rich spectrum of resonant acoustic modes. Based on the solar example
    Antoci, V. et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    66
  • The Dust Environment of Main-Belt Comet P/2010 R2 (La Sagra)
    We present a model of the dust environment of Main-Belt Comet P/2010 R2 (La Sagra) from images acquired during the period 2010 October-2011 January. The tails are best simulated by anisotropic ejection models, with emission concentrated near the nucleus south pole, the spin axis having an obliquity near 90°, indicative of a possible seasonally
    Moreno, F. et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    48
  • Testing the Jet Quenching Paradigm with an Ultradeep Observation of a Steadily Soft State Black Hole
    We present ultradeep radio observations with the Expanded Very Large Array of 4U 1957+11, a Galactic black hole (BH) candidate X-ray binary known to exist in a persistent soft X-ray state. We derive a stringent upper limit of 11.4 μJy beam-1 (3σ) at 5-7 GHz, which provides the most rigorous upper limit to date on the presence of jets in a soft
    Russell, D. M. et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    109
  • Swift observations of the accreting millisecond pulsar IGR J17498-2921: from outburst to quiescence
    Swift has been monitoring the accreting millisecond pulsar IGR J17498-2921 since the start of its outburst in 2011 August 12 (ATels #3551, #3555, #3556). We detected two X-ray bursts on Aug. 18 and 28. During the first ~12 days the average persistent XRT count rate remained approximately constant at 3-7 c/s. Around Aug. 24 the source count rate
    Linares, M. et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    4