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..

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  • Polarimetric observations of a sample of Compact Steep-Spectrum sources
    Measurements of the polarised emission from Compact Steep-Spectrum (CSS) sources can give important information about the physical conditions inside and around the region of radio emission, essentially on the Narrow Line Region. We have observed the sample of CSS sources constructed by Fanti et al. (1990) with the Effelsberg 100-m radio telescope
    Mantovani, F. et al.

    Fecha de publicación:

    2
    2009
    Número de citas
    0
  • Phase-resolved spectroscopy of the accreting millisecond X-ray pulsar SAX J1808.4-3658 during the 2008 outburst
    Aims: We obtained phase-resolved spectroscopy of the accreting millisecond X-ray pulsar SAX J1808.4-3658 during its outburst in 2008 to find a signature of the donor star, constrain its radial velocity semi-amplitude (K_2), and derive estimates for the pulsar mass. Methods: Using Doppler images of the Bowen region, we find a significant (≥8σ)
    Cornelisse, R. et al.

    Fecha de publicación:

    2
    2009
    Número de citas
    14
  • Optimal Filter Systems for Photometric Redshift Estimation
    In the coming years, several cosmological surveys will rely on imaging data to estimate the redshift of galaxies, using traditional filter systems with 4-5 optical broad bands; narrower filters improve the spectral resolution, but strongly reduce the total system throughput. We explore how photometric redshift performance depends on the number of
    Benítez, N. et al.

    Fecha de publicación:

    2
    2009
    Número de citas
    72
  • Optical spectroscopy of V1123 Tauri and its visual companion
    We present long-slit intermediate resolution spectroscopy of the visual binary V1123. We confirm that component A is a W UMa eclipsing star with spectral type G0V, while component B is a K0V. We infer a distance to the system of 125 pc, and then a projected separation between both components of 520 AU. The difference in radial velocities of
    Gutiérrez, Carlos M.

    Fecha de publicación:

    2
    2009
    Número de citas
    2
  • On the origin of dwarf elliptical galaxies: the fundamental plane
    Context: Early-type dwarf (dE) galaxies are the most common type of galaxies observed in the Universe. Their study has important cosmological implications because according to hierarchical galaxy evolution theories they are the progenitors of brighter galaxies. Nevertheless, the origin of this kind of system is still not well understood. Aims: The
    Aguerri, J. A. L. et al.

    Fecha de publicación:

    2
    2009
    Número de citas
    74
  • Neon and Chemical Fractionation Trends in Late-type Stellar Atmospheres
    A survey of Ne, O and Fe coronal abundances culled from the recent literature for about 60 late-type stars confirms that the Ne/O ratio of stellar outer atmospheres is about two times the value recently recommended by Asplund et al. The mean Ne/O remains flat from the most active stars down to at least intermediate activity levels (-5
    García-Alvarez, David et al.

    Fecha de publicación:

    2
    2009
    Número de citas
    8