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/

  • Thesis
    MORFOLOGÍA Y FORMACIÓN ESTELAR DE LAS GALAXIAS EN CÚMULOS CERCANOS
    RUBEN SANCHEZ JANSSEN

    Advertised on:

    7
    2009
  • Refereed
    Mg and TiO spectral features at the near-IR: spectrophotometric index definitions and empirical calibrations
    Using the near-infrared spectral stellar library of Cenarro et al., the behaviour of the MgI line at 8807 Å and nearby TiO bands is analyzed in terms of the effective temperature, surface gravity and metallicity of the library stars. New spectroscopic indices for both spectral features - namely MgI and sTiO - are defined, and their sensitivities to
    Cenarro, A. J. et al.

    Advertised on:

    7
    2009
    Bibcode
    2009MNRAS.396.1895C
    Citations
    21
  • Refereed
    Magnetic field strength of active region filaments
    Aims: We study the vector magnetic field of a filament observed over a compact active region neutral line. Methods: Spectropolarimetric data acquired with TIP-II (VTT, Tenerife, Spain) of the 10 830 Å spectral region provide full Stokes vectors that were analyzed using three different methods: magnetograph analysis, Milne-Eddington inversions, and
    Kuckein, C. et al.

    Advertised on:

    7
    2009
    Bibcode
    2009A&A...501.1113K
    Citations
    79
  • Refereed
    Long-term stability of spotted regions and the activity-induced Rossiter-McLaughlin effect on V889 Herculis. A synergy of photometry, radial velocity measurements, and Doppler imaging
    Context: The young active G-dwarf star V889 Herculis (HD 171488) shows pronounced spots in Doppler images as well as large variations in photometry and radial velocity (RV) measurements. However, the lifetime and evolution of its active regions are not well known. Aims: We study the existence and stability of active regions on the star's surface
    Huber, K. F. et al.

    Advertised on:

    7
    2009
    Bibcode
    2009A&A...501..715H
    Citations
    20