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
    Rubidium-rich asymptotic giant branch stars in the Magellanic Clouds
    Not Available
    García-Hernández, A. et al.

    Fecha de publicación:

    11
    2009
    Bibcode
    2009iac..talk..112G
    Número de citas
    0
  • Sin árbitro
    Response of the solar atmosphere to the photospheric plasma motion
    Not Available
    Büchner, J. et al.

    Fecha de publicación:

    11
    2009
    Bibcode
    2009iac..talk..111B
    Número de citas
    0
  • Sin árbitro
    Relativistic hydro and magnetohydrodynamic models for AGN jet propagation and deceleration
    Not Available
    Keppens, R. et al.

    Fecha de publicación:

    11
    2009
    Bibcode
    2009iac..talk..109K
    Número de citas
    0
  • Con árbitro
    Rb-Rich Asymptotic Giant Branch Stars in the Magellanic Clouds
    We present high-resolution (R ~ 60,000) optical spectra of a carefully selected sample of heavily obscured and presumably massive O-rich asymptotic giant branch (AGB) stars in the Magellanic Clouds. We report the discovery of strong Rb I lines at 7800 Å in four Rb-rich LMC stars at luminosities equal to or greater than the standard adopted
    García-Hernández, D. A. et al.

    Fecha de publicación:

    11
    2009
    Bibcode
    2009ApJ...705L..31G
    Número de citas
    92
  • Con árbitro
    OTELO Survey: Deep BVRI Broadband Photometry of the Groth Strip. II. Optical Properties of X-Ray Emitters
    The Groth field is one of the sky regions that will be targeted by the OSIRIS Tunable Filter Emission Line Object survey in the optical 820 nm and 920 nm atmospheric windows. In the present paper, public Chandra X-ray data with total exposure time of 200 ks are analyzed and combined with optical broadband data of the Groth field, in order to study
    Pović, M. et al.

    Fecha de publicación:

    11
    2009
    Bibcode
    2009ApJ...706..810P
    Número de citas
    25
  • 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