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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  • Converting Hα Luminosities into Star Formation Rates
    Star formation rates (SFRs) of galaxies are commonly calculated by converting the measured Hα luminosities (LHα) into current SFRs. This conversion is based on a constant initial mass function (IMF) independent of the total SFR. As was recently recognized, the maximum stellar mass in a star cluster is limited by the embedded total cluster mass and
    Pflamm-Altenburg, Jan et al.

    Fecha de publicación:

    12
    2007
    Número de citas
    119
  • Coordinated observations of the red dwarf flare star EV Lacertae in 1992.
    Results of coordinated observations of the flare star EV Lac in September 1992 are presented. Among 25 flares detected during 28 hours on patrol in Crimea four had large enough amplitudes to permit the quantitative analysis of their radiation by colour-colour diagrams. Calculation of V-I colour index for different radiation sources enable us to
    Abdul-Aziz, H. et al.

    Fecha de publicación:

    12
    1995
    Número de citas
    34
  • Cophasing of segmented mirrors using the pyramid sensor
    All the projects of the Extremely Large Telescopes (ELTs) are based on segmented primary mirrors. This idea, solving the problem of producing single mirrors having diameter larger than 8m, introduces the needs for an accurate co-phasing of the various segments. The paper presents some laboratory measurements aimed to investigate the use of the
    Esposito, Simone et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    19
  • Correcting the spectroscopic surface gravity using transits and asteroseismology. No significant effect on temperatures or metallicities with ARES and MOOG in local thermodynamic equilibrium
    Context. Precise stellar parameters (effective temperature, surface gravity, metallicity, stellar mass, and radius) are crucial for several reasons, amongst which are the precise characterization of orbiting exoplanets and the correct determination of galactic chemical evolution. The atmospheric parameters are extremely important because all the
    Mortier, A. et al.

    Fecha de publicación:

    12
    2014
    Número de citas
    75
  • Correlations between Structural Parameters of Disk Galaxies
    We have obtained (in BVRI filters) the structural parameters of four disk galaxies, spanning a range of different morphological types. We believe the parameters are reliable because an extensive part of the galaxies' disks are free from contamination by other components, and a detailed photometric method has been used to derive these quantities
    Prieto, Mercedes et al.

    Fecha de publicación:

    12
    1999
    Número de citas
    0
  • Correlations in superstatistical systems
    We review some of the statistical properties of higher-dimensional superstatistical stochastic models. As an example, we analyse the stochastic properties of a superstatistical model of 3-dimensional Lagrangian turbulence, and compare with experimental data. Excellent agreement is obtained for various measured quantities, such as acceleration
    Beck, Christian

    Fecha de publicación:

    12
    2007
    Número de citas
    1