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
    Quasar hosts. A workshop jointly organized by ESO and IAC, Puerto de la Cruz, Tenerife, 24 - 27 Sep 1996.
    Not Available
    Crane, P. et al.

    Fecha de publicación:

    12
    1996
    Bibcode
    1996Msngr..86...39C
    Número de citas
    0
  • Con árbitro
    Quenching cluster cooling flows with recurrent hot plasma bubbles
    The observed cooling rate of hot gas in clusters is much lower than that inferred from the gas density profiles. This suggests that the gas is being heated by some source. We use an adaptive-mesh refinement code (FLASH) to simulate the effect of multiple, randomly positioned, injections of thermal energy within 50 kpc of the centre of an initially
    Dalla Vecchia, C. et al.

    Fecha de publicación:

    12
    2004
    Bibcode
    2004MNRAS.355..995D
    Número de citas
    92
  • Con árbitro
    QUEST1 Variability Survey. II. Variability Determination Criteria and 200k Light Curve Catalog
    The QUEST (QUasar Equatorial Survey Team) Phase 1 camera has collected multibandpass photometry on a large strip of high Galactic latitude sky over a period of 26 months. This robust data set has been reduced and nightly catalogs compared to determine the photometric variability of the ensemble objects. Subsequent spectroscopic observations have
    Rengstorf, A. W. et al.

    Fecha de publicación:

    12
    2004
    Bibcode
    2004ApJ...617..184R
    Número de citas
    20
  • Con árbitro
    Quiescent X-ray/optical counterparts of the black hole transient H 1705-250
    We report the result of a new Chandra observation of the black hole X-ray transient H 1705-250 in quiescence. H 1705-250 was barely detected in the new ˜50 ks Chandra observation. With five detected counts, we estimate the source quiescent luminosity to be LX ˜ 9.1 × 1030 erg s-1 in the 0.5-10 keV band (adopting a distance of 8.6 kpc). This value
    Wijnands, R. et al.

    Fecha de publicación:

    12
    2012
    Bibcode
    2012MNRAS.427.2876Y
    Número de citas
    10
  • Sin árbitro
    Quiet Solar Photosphere: Comparisons of High Resolution Observations with 3-D Simulations
    Not Available
    Cauzzi, G. et al.

    Fecha de publicación:

    12
    2005
    Bibcode
    2005ESASP.600E..12C
    Número de citas
    0