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/

  • Clues to Substellar Formation: Rotation and the Low-Mass End of the Initial Mass Function
    We have monitored S Ori 45, a young, low-mass (20 M j up) brown dwarf of the σ Orionis cluster (˜3 Myr, 352 pc), using optical and near-infrared filters. S Ori 45 (spectral type M8.5) is found to be multi-periodic with a dominant modulation at 2.5 3.5 h, and a short modulation at about 46 min. We ascribe the longer of these modulations to a
    Zapatero Osorio, María Rosa et al.

    Advertised on:

    8
    2004
    Citations
    3
  • Chemical Abundances of the Galactic H II Region NGC 3576 Derived from Very Large Telescope Echelle Spectrophotometry
    We present echelle spectrophotometry of the Galactic H II region NGC 3576. The data have been taken with the VLT UVES echelle spectrograph in the 3100-10400 Å range. We have measured the intensities of 458 emission lines, 344 are permitted lines of H0, He0, C+, N0, N+, N++, O0, O+, Ne+, S++, Si0, Si+, Ar0, and Ar+; some of them are produced by
    García-Rojas, Jorge et al.

    Advertised on:

    8
    2004
    Citations
    107
  • Book Review: Cosmochemistry. The melting pot of the elements / C. Esteban R. J. G. López, A. Herrero, F. Sánchez (eds.). Cambridge, Cambridge University Press, 2004, XII+298 pp., ISBN 0-521-82768-X
    Not Available
    Esteban, C. et al.

    Advertised on:

    8
    2004
    Citations
    0
  • Analysis of Simultaneous Visible and Infrared Spectropolarimetric Observations of Quiet Sun
    Not Available
    Domínguez Cerdeña, Itahiza et al.

    Advertised on:

    8
    2004
    Citations
    0
  • a Relief to the Supersymmetric Fine Tuning Problem
    As is well known, electroweak breaking in the MSSM requires substantial fine-tuning. We explain why this fine tuning problem is abnormally acute, and this allows to envisage possible solutions to this undesirable situation. Following these ideas, we review some recent work which shows how in models with SUSY broken at a low scale (not far from the
    Casas, J. A. et al.

    Advertised on:

    8
    2004
    Citations
    15