Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Refereed
    On emission-line spectra obtained from evolutionary synthesis models. II. Scale-relations and the estimation of mass dependences
    Aims: In this paper we study the influence of the ionizing cluster mass on the emission line spectrum of H ii regions in order to determine the influence of low mass clusters on the integrated emission line spectra of galaxies. Methods: For this purpose, we present a grid of photoionization models that covers metallicities from Z = 0.001 to Z = 0
    Villaverde, M. et al.

    Advertised on:

    7
    2010
    Bibcode
    2010A&A...517A..93V
    Citations
    8
  • Refereed
    Observations, compositional, and physical characterization of near-Earth and Mars-crosser asteroids from a spectroscopic survey
    Aims: We analyse a significantly large sample of spectroscopic data to provide a compositional characterization of the near-Earth asteroid population. We present visible and near-infrared spectra of a total of 74 near-Earth asteroids (NEAs) and Mars-crossers (MCs), covering the wavelength region from 0.5 to 2.5 μm. Using spectra of NEAs from other
    de León, J. et al.

    Advertised on:

    7
    2010
    Bibcode
    2010A&A...517A..23D
    Citations
    101
  • Thesis
    OBJETOS SUBESTELARES EN CÚMULOS ABIERTOS
    GABRIEL BIHAIN

    Advertised on:

    7
    2010
  • Thesis
    NUCLEOS DE GALAXIAS ACTIVAS A ESCALAS DE PARSECS
    JUAN ANTONIO FERNANDEZ ONTIVEROS

    Advertised on:

    7
    2010
  • Non-refereed
    NEFER: a high-resolution scanning Fabry-Perot Spectrograph II scanning Fabry-Perot testing
    NEFER (Nuevo Espectrómetro Fabry-Perot de Extrema Resolución) is a high spectral resolution, scanning Fabry-Perot Spectrometer. It will be installed in the OSIRIS instrument at the GTC 10 m telescope. This 3D instrument uses a high order scanning Fabry-Perot to obtain highly accurate kinematical information of extended cosmic sources such as
    Bernal, Abel et al.

    Advertised on:

    7
    2010
    Bibcode
    2010SPIE.7735E.155B
    Citations
    0