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 dust masses of powerful radio galaxies: clues to the triggering of their activity
    We use deep Herschel Space Observatory observations of a 90 per cent complete sample of 32 intermediate-redshift 2Jy radio galaxies (0.05 z 0.7) with strong emission lines to estimate the dust masses of their host galaxies and thereby investigate the triggering mechanisms for their quasar-like AGN. The dust masses derived for the radio galaxies
    Tadhunter, C. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    32
  • The Cocoon nebula and its ionizing star: do stellar and nebular abundances agree?
    Context. Main-sequence massive stars embedded in an H ii region should have the same chemical abundances as the surrounding nebular gas+dust. The Cocoon nebula (IC 5146), a close-by Galactic H ii region ionized by a narrow line B0.5 V single star (BD+46 3474), is an ideal target to compare nebular and stellar abundances in detail in the same
    García-Rojas, J. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    27
  • Synthetic Observations of Wave Propagation in a Sunspot Umbra
    Spectropolarimetric temporal series from Fe I λ6301.5 Å and Ca II infrared triplet lines are obtained by applying the Stokes synthesis code NICOLE to a numerical simulation of wave propagation in a sunspot umbra from MANCHA code. The analysis of the phase difference between Doppler velocity and intensity core oscillations of the Fe I λ6301.5 Å line
    Felipe, T. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    28
  • Suppression of cooling by strong magnetic fields in white dwarf stars
    Isolated cool white dwarf stars more often have strong magnetic fields than young, hotter white dwarfs, which has been a puzzle because magnetic fields are expected to decay with time but a cool surface suggests that the star is old. In addition, some white dwarfs with strong fields vary in brightness as they rotate, which has been variously
    Valyavin, G. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    58
  • STELLAR POPULATIONS AND KINEMATICS OF THE FORNAX DSPH GALAXY
    La formación de galaxias y su evolución es a día de hoy una cuestión por resolver. En el escenario Lambda-CDM, las galaxias enanas son los componentes básicos de los cuales se forman las galaxias más grandes. Las enanas que observamos hoy en día podrían ser sistemas supervivientes que todavía no se han fusionado con galaxias más grandes y pueden
    Andrés del Pino Molina

    Fecha de publicación:

    11
    2014
  • Stellar occultation by (119951) 2002 KX14 on April 26, 2012
    Context. Trans-Neptunian objects (TNOs) are important bodies, but very little is known about their basic physical properties such as size, density, and albedo. Aims: We intend to determine sizes, albedos, and even densities of a good sample of TNOs, especially those of the largest TNOs because they can be studied the best with different
    Alvarez-Candal, A. et al.

    Fecha de publicación:

    11
    2014
    Número de citas
    15