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

  • Sin árbitro
    CL-Spectral Characteristics of Quartz and Feldspars in Fresh and Hydrothermal Altered Volcanic Rocks (Cabo de Gata, Almeria, Spain)
    Not Available
    Aparicio, A. et al.

    Fecha de publicación:

    5
    2011
    Bibcode
    2011LPICo1616....3A
    Número de citas
    0
  • Sin árbitro
    Chandra Watches Over A Decade Of Variability In M31 Globular Clusters
    The central region of M31 has been monitored with Chandra > 120 times over the last 11 years. In this region we find X-ray sources corresponding to 35 out of 420 globular clusters; these are highly likely to be X-ray binaries. We have created long-term, calibrated lightcurves for all 35 sources, and will present highlights of our variability survey
    Barnard, Robin et al.

    Fecha de publicación:

    5
    2011
    Bibcode
    2011AAS...21812202B
    Número de citas
    0
  • Sin árbitro
    Candidate optical counterparts of MAXI J1543-564
    We report on optical observations of the field of the black hole candidate X-ray binary MAXI J1543-564 (ATel #3330, #3331, #3334, #3336, #3341, #3355) with the 2-m Faulkes Telescope South (located at Siding Spring, Australia). Three images were acquired in SDSS i'-band on 2011 May 11th, 14th and 15th (MJD 55692.585, 55695.757 and 55696.752)
    Russell, D. M. et al.

    Fecha de publicación:

    5
    2011
    Bibcode
    2011ATel.3359....1R
    Número de citas
    6
  • Con árbitro
    Astrophysical Parameters of LS 2883 and Implications for the PSR B1259-63 Gamma-ray Binary
    Only a few binary systems with compact objects display TeV emission. The physical properties of the companion stars represent basic input for understanding the physical mechanisms behind the particle acceleration, emission, and absorption processes in these so-called gamma-ray binaries. Here we present high-resolution and high signal-to-noise
    Negueruela, Ignacio et al.

    Fecha de publicación:

    5
    2011
    Bibcode
    2011ApJ...732L..11N
    Número de citas
    118