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/

  • Metallicity Estimation Using N2 Method with OSIRIS
    The OTELO (OSIRIS Tunable Emission Line Object Survey project) is an emission line survey using the OSIRIS Tunable Filters on the GTC 10.4m telescope (Cepa et al. 2008). Observing in selected atmospheric windows relatively free of sky emission lines, and with a total survey area of 0.1square degree distributed in different fields, it is expected to
    Lara-López, M. A. et al.

    Advertised on:

    2010
    Citations
    0
  • 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.

    Advertised on:

    2010
    Citations
    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.

    Advertised on:

    2010
    Citations
    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.

    Advertised on:

    2010
    Citations
    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.

    Advertised on:

    2010
    Citations
    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.

    Advertised on:

    2010
    Citations
    0