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

  • The supergiant optical counterpart of ULX P13 in NGC 7793
    We have identified the optical counterpart of the ULX source P13 in the nearby spiral galaxy NGC 7793. The object is a V ˜ 20.5 mag star, ten times brighter than any other established counterpart of a ULX in nearby galaxies. Medium resolution optical spectroscopy carried out in 2008 and 2009 with the ESO-VLT reveals the presence of narrow high
    Motch, C. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    53
  • The Solar Rotation and its Evolution During Cycle 23
    We present the most exhaustive and accurate inferences of the internal solar rotation rate and its evolution during solar cycle 23. A full solar cycle of MDI observations have been analyzed using our state of the art fitting methodology. Time series of various lengths have been fitted, from a single 4608-day long epoch (64 times 72 day or 12.6 yr)
    Korzennik, Sylvain G. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    0
  • The shortest period detached binary white dwarf system
    We identify SDSS J010657.39-100003.3 (hereafter J0106-1000) as the shortest period detached binary white dwarf (WD) system currently known. We targeted J0106-1000 as part of our radial velocity programme to search for companions around known extremely low-mass (ELM; ˜0.2 M&sun;) WDs using the 6.5-m Multiple Mirror Telescope. We detect peak-to-peak
    Kilic, Mukremin et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    47
  • The pathways of C: from AGB stars, to the Interstellar Medium, and finally into the protoplanetary disk
    The origin, and role of C in the formation of first solar system aggregates is described. Stellar grains evidence demonstrates that Asymptotic Giant Branch (AGB) stars were nearby to the solar nebula at the time of solar system formation. Such stars continue to burn H and He in shells that surround the C-O core. During their evolution, flashes
    Trigo-Rodriguez, J. M. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    0
  • The new carbon symbiotic star IPHAS J205836.43+503307.2
    Aims: We are performing a search for symbiotic stars using IPHAS, the INT Hα survey of the northern Galactic plane, and follow-up observations. Methods: Candidate symbiotic stars are selected on the basis of their IPHAS and near-IR colours, and spectroscopy and photometry are obtained to determine their nature. We present here observations of the
    Corradi, R. L. M. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    11
  • The major atmospheric gamma-ray imaging Cherenkov telescope
    MAGIC is a system of two 17 m diameter Imaging Atmospheric Cherenkov Telescopes (IACTs) for ground-based γ-ray astronomy. During many years, starting with the design phase of the first telescope in 2003, the upgrade of the second telescope in 2008 up to now, novel technologies have been developed, commissioned and continuously improved. Most
    Garczarczyk, M. et al.

    Fecha de publicación:

    5
    2011
    Número de citas
    2