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

  • Metallicity Estimates with SDSS-DR6
    We present a study of the metallicity of 20268 galaxies from the Sloan Digital Sky Survey—Data Release 6 (SDSS-DR6)—using the R 23 method, and derive analytical calibrations from several metallicity-sensitive line ratios: [Nii] λ6583/Hα, [Oiii] λ5007/[Nii] λ6583, [Nii] λ6583/[Oii] λ3727, [Nii] λ6583/ [Sii] λλ6717, 6731, [Sii] λλ6717, 6731/Hα, and
    Lara-López, M. A. et al.

    Fecha de publicación:

    2010
    Número de citas
    0
  • Mechanisms Producing Fissionlike Binary Fragments in Heavy Ion Collisions
    The mixing of the quasifission component to the fissionlike cross section causes ambiguity in the quantitative estimation of the complete fusion cross section from the observed angular and mass distributions of the binary products. We show that the partial cross section of quasifission component of binary fragments covers the whole range of the
    Nasirov, Avazbek et al.

    Fecha de publicación:

    2010
    Número de citas
    3
  • Massive Stars with Weak Winds
    The theory of radiatively-driven winds successfully explains the key points of the stellar winds of hot massive stars. However, it has been recently found that some O- and B-type stars do not exhibit as strong wind as predicted by theory. In this work we explain the main issues concerning this topic. We also describe our analysis of the UV spectra
    García, M. et al.

    Fecha de publicación:

    2010
    Número de citas
    0
  • Marco Polo: Hunting and Capture of Material from a Primitive Asteroid
    A description of the Spanish contribution to the Marco Polo mission and of the mission itself is presented. Marco Polo is a joint European-Japanese mission of sample return from a Near Earth Object (NEO). Submitted to ESA on July 2007 in the framework of the Cosmic Vision 2015-2025, Marco Polo passed the first evaluation process on October 2007
    Licandro, J.

    Fecha de publicación:

    2010
    Número de citas
    0
  • Magnetic Fingerprints of Solar and Stellar Oscillations
    Waves connect all the layers of the Sun, from its interior to the upper atmosphere. It is becoming clear now the important role of magnetic field on the wave propagation. Magnetic field modifies propagation speed of waves, thus affecting the conclusions of helioseismological studies. It can change the direction of the wave propagation, help
    Khomenko, E.

    Fecha de publicación:

    2010
    Número de citas
    0
  • Low-Degree High-Frequency p and g Modes in the Solar Core
    Solar gravity (g) modes propagate within the radiative part of the solar interior and are highly sensitive to the physical conditions of the solar core. They would represent the best tool to infer the structure and the dynamics of the radiative interior, in particular the core, if they were properly detected and characterized. Although individual
    Mathur, S. et al.

    Fecha de publicación:

    2010
    Número de citas
    0