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
    On the Origin of the IR Emission in Active Galactic Nuclei
    The relation between the X-ray, coronal line and IR emission in a sample of the brightest known Seyfert galaxies is analyzed. A close relationship between the absorption-corrected soft X-ray emission and both the mid-IR and the coronal line emission is found for the Seyfert 2-type objects in the sample. The coronal line and X-ray emission both
    Almudena Prieto, M. et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001ASPC..249..263A
    Número de citas
    0
  • Sin árbitro
    Nuclear Star Formation in the Hotspot Galaxy NGC 2903
    We analyze the star formation properties of the hotspot galaxy NGC 2903 using high resolution Hubble Space Telescope and adaptive optics observations. The circumnuclear star formation in NGC 2903 shows a ringlike morphology with an approximate diameter of 625 pc. For the first time, the infrared hotspots have been resolved into individual young
    Alonso-Herrero, A. et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001ASPC..249..557A
    Número de citas
    0
  • Sin árbitro
    Nuclear Components in the Bulges of Disk Galaxies
    By combining surface brightness profiles from images taken in the HST/NICMOS F160W and ground-based K bands, we have obtained NIR profiles for a well studied sample of inclined disk galaxies, spanning radial ranges from 20 pc to a few kpc. We fit PSF-convolved Sersic-plus-exponential laws to the profiles, and compare the results with the fits to
    Balcells, Marc et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001ASPC..249..167B
    Número de citas
    6
  • Sin árbitro
    Non-LTE inversion of spectral lines and Stokes profiles (Invited Review)
    Not Available
    Socas-Navarro, H.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001hsa..conf..233S
    Número de citas
    0
  • Sin árbitro
    Non-linear Effects in Pulsating White Dwarfs
    Asteroseismology is a very powerful technique to study the interior of pulsating stars like the ZZ Ceti white dwarfs (DAV), because the driving mechanism is strongly correlated with the chemical composition of the layers in the star. The necessary first step is the identification of the pulsation mode. In contrast to our sun most DA variables (H
    Weidner, C. et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001AGM....18.P113W
    Número de citas
    0