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

  • Con árbitro
    Optical studies of V404 Cyg, the X-ray transient GS 2023+338. IV. The rotation speed of the companion star.
    Not Available
    Casares, J. et al.

    Fecha de publicación:

    11
    1994
    Bibcode
    1994MNRAS.271L...5C
    Número de citas
    118
  • Con árbitro
    Optical variability of the ultracool dwarf TVLM 513-46546: evidence for inhomogeneous dust clouds
    We present multicolour photometry of the M8.5V ultracool dwarf `pulsar' TVLM 513-46546 (hereafter TVLM 513) obtained with the triple-beam photometer ULTRACAM. Data were obtained simultaneously in the Sloan-g' and Sloan-i' bands. The previously reported sinusoidal variability, with a period of 2 h, is recovered here. However, the Sloan-g' and Sloan
    Littlefair, S. P. et al.

    Fecha de publicación:

    11
    2008
    Bibcode
    2008MNRAS.391L..88L
    Número de citas
    33
  • Con árbitro
    Orbital periods of cataclysmic variables identified by the SDSS. VI. The 4.5-h period eclipsing system SDSS J100658.40+233724.4
    We present time-resolved spectroscopy and photometry of SDSS J100658.40+233724.4, which we have discovered to be an eclipsing cataclysmic variable with an orbital period of 0.18591324 days (267.71507 min). The observed velocity amplitude of the secondary star is 276 ± 7 km s-1, which an irradiation correction reduces to 258 ± 12 km s-1. Doppler
    Southworth, J. et al.

    Fecha de publicación:

    11
    2009
    Bibcode
    2009A&A...507..929S
    Número de citas
    29
  • Sin árbitro
    Origin and fate of the most massive galaxies
    In the last five years there has been cumulative evidence showing that massivegalaxies have dramatically grown in size since z ˜ 3. This result hasremained very controversial as it seems at odd with our previous knowledgebased on the detailed analysis of the stellar populations of nearby massivegalaxies which shows that their stars were form very
    Trujillo, I.

    Fecha de publicación:

    11
    2011
    Bibcode
    2011hsa6.conf..120T
    Número de citas
    0
  • Sin árbitro
    Origin of space and time in a non-commutative cosmological model
    Not Available
    Hernandez-Monteagudo, C.

    Fecha de publicación:

    11
    2008
    Bibcode
    2008iac..talk...35H
    Número de citas
    0