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

  • An Imaging Survey of Nearby Spiral Galaxies
    We describe the progress of a large optical and near-infrared imaging study of a complete sample of 57 spiral galaxies. We have obtained B, I, K' and Hα imaging to map stellar populations and massive star formation (SF) across the arm and interarm regions, in order to study the distribution of mass and SF in these different and distinct
    Knapen, J. H. et al.

    Fecha de publicación:

    12
    2002
    Número de citas
    0
  • An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). IV. Discovery of High-redshift AGB Analogs
    The survey for DUST in Nearby Galaxies with Spitzer (DUSTiNGS) identified several candidate Asymptotic Giant Branch (AGB) stars in nearby dwarf galaxies and showed that dust can form even in very metal-poor systems ({\boldsymbol{Z}}∼ 0.008 {Z}ȯ ). Here, we present a follow-up survey with WFC3/IR on the Hubble Space Telescope (HST), using filters
    Boyer, M. L. et al.

    Fecha de publicación:

    12
    2017
    Número de citas
    45
  • An Intensive HST, IUE, and Ground-Based Study of NGC 5548
    We present the first results of a combined HST/IUE/ground-based spectroscopic monitoring campaign on the Seyfert 1 galaxy NGC 5548 that was undertaken in order to address questions that require both higher temporal resolution and higher signal-to-noise ratios than were obtained in our previous multiwavelength monitoring of this galaxy in 1988 -- 89
    Korista, K. T. et al.

    Fecha de publicación:

    12
    1994
    Número de citas
    0
  • An observational approach to convection in main sequence stars
    Observational results concerning possible changes in the granulation of Main Sequence stars were found by analysing their seismic power spectra obtained from photometric microvariability. We analysed as many as 178 stars with spectral types F, G, K, and M observed for 54 days. We present evidence of changes in the lifetime and contrast of the
    Régulo, C. et al.

    Fecha de publicación:

    12
    2005
    Número de citas
    3
  • An Optimized H_β Index for Disentangling Stellar Clusters and Galaxy Ages
    We have derived a new H_{β} absorption index definition, which is fully optimized as an age indicator for old and intermediate-aged stellar populations. Rather than using stellar spectra, we employed theoretical SEDs at moderately high resolution for simple stellar populations of different ages and metallicities. The new index, which is virtually
    Cervantes-Rodriguez, J. L. et al.

    Fecha de publicación:

    12
    2007
    Número de citas
    0
  • An Umbral Brightening Associated with a Two-Ribbon Flare
    We report an unusual case of a two-ribbon flare associated with an umbral brightening in a magnetically unipolar region.
    Vazquez, M. et al.

    Fecha de publicación:

    12
    1979
    Número de citas
    1