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/

  • 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
  • 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.

    Advertised on:

    2010
    Citations
    0
  • Kinematics of Inner Bars. The Stellar σ-Hollows
    We present SAURON stellar kinematical analysis for four double-barred early-type galaxies: NGC 2859, NGC 3941, NGC 4725 and NGC 5850. The presence of the inner bar is not evident from the radial velocity, but it appears to have an important effect in the stellar velocity dispersion maps: we find two σ-hollows of amplitudes between 10 and 40 km s- 1
    de Lorenzo-Cáceres, A. et al.

    Advertised on:

    2010
    Citations
    0
  • Interior and Exterior Clues of Solar Activity
    Two research paths are described to obtain better understanding of the origin of global solar activity. First, observations with a multichannel resonant spectrometer may reveal the dynamics of the solar core, the tachocline, and the temporal evolution of activity between the photosphere and chromosphere. Such new observations will deliver
    Turck-Chièze, S. et al.

    Advertised on:

    2010
    Citations
    0