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

  • MAXI J1305-704: Optical Spectroscopy with SALT
    We report on optical spectroscopy of the black hole candidate MAXI J1305-704 (ATel #4024; #4030) using SALT and the Robert Stobie Spectrograph. On 2012 April 15 (20:40-23:00 UTC) and 16 (22:30-01:40 UTC) we obtained 2 hrs of continuous spectroscopy using a slit width of 0.6 arcsec, resulting in a wavelength coverage of 4050-5100 Angstrom and a
    Charles, Phil et al.

    Fecha de publicación:

    5
    2012
    Número de citas
    3
  • Mass ratio from Doppler beaming and Rømer delay versus ellipsoidal modulation in the Kepler data of KOI-74
    We present a light-curve analysis and radial velocity study of KOI-74, an eclipsing A star + white dwarf binary with a 5.2-d orbit. Aside from new spectroscopy covering the orbit of the system, we used 212 d of publicly available Kepler observations and present the first complete light-curve fitting to these data, modelling the eclipses and
    Bloemen, S. et al.

    Fecha de publicación:

    5
    2012
    Número de citas
    49
  • Manganese in dwarf spheroidal galaxies
    We provide manganese abundances (corrected for the effect of the hyperfine structure) for a large number of stars in the dwarf spheroidal galaxies Sculptor and Fornax, and for a smaller number in the Carina and Sextans dSph galaxies. Abundances had already been determined for a number of other elements in these galaxies, including α and iron-peak
    North, P. et al.

    Fecha de publicación:

    5
    2012
    Número de citas
    50
  • Main Belt Comets: Status Report of the Monitoring Large Programme at ESO
    A status report of the 4-years long ESO Large Program, aimed at monitoring and characterizing Main Belt Comets. The program is 50% completed. Some of the MBCs were observed active. In some cases, the dust is the aftermath of an impact.
    Hainaut, O. R. et al.

    Fecha de publicación:

    5
    2012
    Número de citas
    0