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/

  • Non-refereed
    First Observational Evidences for the Presence of Active, Localized Magnetic Structures in White Dwarfs
    The magnetic white dwarf WD 1953-011 demonstrates the presence of two-component magnetic field geometry in photosphere. The geometry consists of a weak, large-scale component, and a strong, localized component (magnetic ``spot''). The localized component of the field is derived from variable due to the star's rotation circular polarization and
    Valyavin, G. et al.

    Advertised on:

    0
    2011
    Bibcode
    2011mast.conf..295V
    Citations
    1
  • Non-refereed
    Field test of the hybrid photodetector R9792U-40 on the MAGIC camera
    The hybrid photodetector (HPD) R9792U-40 has very high peak quantum efficiency ($>50$% at 500 nm), excellent charge resolution and very low after-pulsing probability (500 times less than that of currently used photomultipliers (PMTs)). These features will improve the sensitivity, the energy resolution and the energy threshold of the MAGIC telescope
    Saito, Takayuki

    Advertised on:

    0
    2011
    Bibcode
    2011ICRC....9..214S
    Citations
    0
  • Refereed
    Extra line-broadening in O-type stars
    Using original data and incorporating similar data from previous studies we investigated the effect of extra line-broadening in the atmosphere of Galactic O-stars. Our results suggest that if not taken into account, the extra broadening can lead to significant overestimation of the measured v sin i. The effect is not large (less than 30 kms), and
    Markova, N. et al.

    Advertised on:

    0
    2011
    Bibcode
    2011BlgAJ..17...54M
    Citations
    2
  • Non-refereed
    Do All O Stars Form in Star Clusters?
    The question whether or not massive stars can form in isolation or only in star clusters is of great importance for the theory of (massive) star formation as well as for the stellar initial mass function of whole galaxies (IGIMF-theory). While a seemingly easy question it is rather difficult to answer. Several physical processes (e.g. star-loss due
    Weidner, C. et al.

    Advertised on:

    0
    2011
    Bibcode
    2011sca..conf..264W
    Citations
    2