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
    Automatic classification of optical sources candidates to be in the post-AGB stage
    Not Available
    Suárez, O. et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001hsa..conf..229S
    Número de citas
    0
  • Sin árbitro
    Asteroseismology in the Main Sequence: The δ Scuti Stars of Praesepe Cluster (CD-ROM Directory: contribs/hernand)
    Not Available
    Hernández, M. M. et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001ASPC..223.1426H
    Número de citas
    0
  • Sin árbitro
    Anisotropy in the mid-IR emission of Seyfert galaxies
    Based on Mid and far-IR data of a complete set of Seyfert galaxies we analyse the Spectral Energy Distributions (SED) of these objects. These SEDs can be separated into three thermal emission components. This separation can be used to introduce some sort of spatial resolution in the inherently low resolution ISO data. It can also be applied as a
    Pérez Garcia, A. M. et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001qhte.conf..255P
    Número de citas
    0
  • Sin árbitro
    An Iceberg Scenario for Late-Type Spiral Galaxy Bulges
    Fitting exponential profiles to the bulges of the early-type spiral galaxies from de Jong & van der Kruit (1994) under-estimates their sizes at the 2-3 sigma significance level. Allowing for the range of structural shapes which these bulges possess - through fitting an r1/n profile - the mean effective bulge radius to disk scale-length ratio, re/h
    Graham, A. W. et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001ASPC..230..103G
    Número de citas
    1
  • Sin árbitro
    Advantages of NIR Multiobject Spectroscopy of z ˜ 1 Galaxies
    Galaxy redshift surveys from z ˜ 1 to z ˜ 4 providing thousands of identified objects are already available. Only for a small and selected sample of those galaxies, near-infrared (NIR) spectroscopy and emission line studies exist. This is mainly due to the time-consuming work of observing one object at a time. This will change with the advent of
    Domínguez-Tagle, Carlos et al.

    Fecha de publicación:

    0
    2001
    Bibcode
    2001defi.conf..153D
    Número de citas
    0