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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  • What Is the Redshift of the Gamma-ray BL Lac Source S4 0954+65?
    High signal-to-noise ratio spectroscopic observations of the BL Lac object S4 0954+65 at the alleged redshift z = 0.367 are presented. This source was detected at gamma frequencies by the MAGIC (TeV) and FERMI (GeV) telescopes during a remarkable outburst that occurred in 2015 February, making the determination of its distance particularly relevant
    Landoni, M. et al.

    Fecha de publicación:

    12
    2015
    Número de citas
    27
  • Wide-field Precision Kinematics of the M87 Globular Cluster System
    We present the most extensive combined photometric and spectroscopic study to date of the enormous globular cluster (GC) system around M87, the central giant elliptical galaxy in the nearby Virgo Cluster. Using observations from DEIMOS and the Low Resolution Imaging Spectrometer at Keck, and Hectospec on the Multiple Mirror Telescope, we derive new
    Strader, Jay et al.

    Fecha de publicación:

    12
    2011
    Número de citas
    161
  • Widely separated binary systems of very low-mass stars
    In this paper we review some recent detections of wide binary brown dwarf systems and discuss them in the context of the multiplicity properties of very low-mass stars and brown dwarfs.
    Phan-Bao, N. et al.

    Fecha de publicación:

    12
    2005
    Número de citas
    0
  • Wind Accretion and State Transitions in the Black Hole Binary Cyg X-1
    The black hole binary, Cyg X-1, is generally observed in one of two long duration X-ray states: a low flux, hard spectrum state (most common) and a high flux, soft spectrum state (rare). Models predict that the high/ soft state corresponds to a high mass transfer phase in the binary, and since the X-ray source is fueled by accretion from the
    Gies, D. R. et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    0
  • Wind variability of LBV stars
    General properties of Luminous Blue Variables (LBV) have been reviewed by Lamers (1987). The LBV's are all close to the Humphreys-Davidson luminosity upper limit. The semi periods of the photometric microvariations with Delta V is about 0.1m are about twice as large as for normal supergiants of the same L and Teff, and 4-20 times larger than the
    Israelian, G. L.

    Fecha de publicación:

    12
    1993
    Número de citas
    0
  • Winds Driven by Super-Star Clusters
    Here we present a self-consistent stationary solution for spherically symmetric winds driven by massive star clusters under the impact of radiative cooling. We demonstrate that cooling may modify drastically the distribution of temperature if the rate of injected energy approaches a critical value and that the stationary wind solution does not
    Silich, S. et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    0