Tipo de publicación: Sin árbitro

  • Publicación
    The plague of magnetic spots among the hot stars of globular clusters: a bridge between MS and WD stars
    I will report on our recent discovery of a wide-spread photometric variability among hot (~20,000 – 30,000 K) extreme horizontal branch (EHB) stars in Galactic...
  • Publicación
    The plague of magnetic spots among the hot stars of globular clusters: a bridge between MS and WD stars
    I will report on our recent discovery of a wide-spread photometric variability among hot (~20,000 – 30,000 K) extreme horizontal branch (EHB) stars in Galactic...
  • Publicación
    The Planck mission: Early Results
    Not Available
  • Publicación
    The planetary nebula NGC 6153 through the eyes of MUSE
    In this contribution, we present the results of a study on the high abundance discrepancy factor (ADF $\sim$ 10) planetary nebula (PN) NGC 6153 with MUSE. We...
  • Publicación
    The planetary nebulae in NGC6822 revisited
    Spectroscopic data for 20 PNe in the irregular galaxy NGC6822 have been studied. This represents 80% of the total sample of PNe candidates in this galaxy. We...
  • Publicación
    The planetary system of Proxima Centauri seen with ESPRESSO
    During last decade there have been a tremendous increase in detection and characterization of low-mass exoplanets, reaching the Earth size and mass domain, in...
  • Publicación
    The PLATO 2.0 mission. Spanish contribution
    The PLATO 2.0 space mission (PLAnetary Transits and Oscillation of stars) was selected by the ESA Science Programme in February 2014, as the M3 mission to be...
  • Publicación
    The plenoptic camera as a wavefront sensor for the European Solar Telescope (EST)
    The plenoptic wavefront sensor combines measurements at pupil and image planes in order to obtain wavefront information from different points of view...
  • Publicación
    The polarization of the Hα line in the quiet solar chromosphere
    One-dimensional radiative transfer (RT) calculations suggested that the scattering polarization profiles of the Hα line are very sensitive to the strength and...