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

  • Circumstellar disc geometry constrained by infrared line fluxes
    Lenorzer et al. introduce ratios of hydrogen infrared recombination lines as a diagnostic tool to constrain the spatial distribution and physical condition of circumstellar material around hot massive stars. They demonstrate that the observed line flux ratios Hu14/Brα and Hu14/Pfγ from different types of objects associated with circumstellar
    Jones, C. E. et al.

    Fecha de publicación:

    1
    2009
    Número de citas
    13
  • Characterization of Active Galactic Nuclei and Their Hosts in the Extended Groth Strip: A Multiwavelength Analysis
    We have employed a reliable technique of classification of active galactic nuclei (AGNs) based on the fit of well sampled spectral energy distributions (SEDs) with a complete set of AGN and starburst galaxy templates. We have compiled UV, optical, and IR data for a sample of 116 AGNs originally selected for their X-ray and mid-IR emissions (96 with
    Ramos Almeida, C. et al.

    Fecha de publicación:

    1
    2009
    Número de citas
    9
  • Black Hole Physics and Strong Gravity with IXO
    Studies of black holes are at a threshold. There is compelling evidence for the existence of both stellar-mass and supermassive black holes, and research is now focused on determining their properties and environmental effects. Most importantly, we are starting to realize the long-held promise of black holes as the ultimate laboratories for
    Brenneman, Laura et al.

    Fecha de publicación:

    1
    2009
    Número de citas
    0
  • Azimuthal dependence of the density distribution in outer galactic discs accreting intergalactic flows
    Aims: The amplitude and scaleheight of the Galactic gas disc density are not axisymmetric against expectations in a self-gravity axisymmetric disc. However, this lopsidedness can be explained in terms of intergalactic accretion flows, which produce non-axisymmetric pressure on the disc. This mechanism could be also responsible for the formation of
    López-Corredoira, M. et al.

    Fecha de publicación:

    1
    2009
    Número de citas
    6
  • An optimized Hβ index for disentangling stellar population ages
    We have defined a new Hβ absorption index definition, Hβo, which has been optimized as an age indicator for old and intermediate age stellar populations. Rather than using stellar spectra, we employed for this purpose a library of stellar population spectral energy distributions of different ages and metallicities at moderately high resolution. Hβo
    Cervantes, J. L. et al.

    Fecha de publicación:

    1
    2009
    Número de citas
    70
  • A Shift in Jupiter's Equatorial Haze Distribution Imaged with the Multi-Conjugate Adaptive Optics Demonstrator at the VLT
    Jupiter was imaged during the Science Demonstration of the MCAO Demonstrator (MAD) at the European Southern Observatory's Very Large Telescope. Io and Europa were used as natural guide stars on either side of Jupiter, separated from each other by about 1.6 arcmin from 23:41 to 01:32 UT (2008 Aug 16/17). The corrected angular resolution was 0.090
    Wong, Michael H. et al.

    Fecha de publicación:

    1
    2009
    Número de citas
    1