Publication type: Refereed

  • Publication
    The Magellanic Clouds as a Template for the Study of Stellar Populations and Galaxy Interactions
    The Magellanic System represents one of the best places to study the formation and evolution of galaxies. Photometric surveys of various depths, areas and...
  • Publication
    The MAGellanic Inter-Cloud (MAGIC) project - II. Slicing up the Bridge
    The origin of the gas in between the Magellanic Clouds (MCs), known as the Magellanic Bridge, has always been the subject of controversy. To shed light into...
  • Publication
    The Magellanic Inter-Cloud Project (MAGIC) III: first spectroscopic evidence of a dwarf stripping a dwarf
    The Magellanic Bridge (MB) is a gaseous stream that links the Large (LMC) and Small (SMC) Magellanic Clouds. Current simulations suggest that the MB forms from...
  • Publication
    The MAGellanic Inter-Cloud Project (MAGIC). I. Evidence for Intermediate-age Stellar Populations in between the Magellanic Clouds
    The origin of the gas in between the Magellanic Clouds (MCs)—known as the "Magellanic Bridge" (MB)—is puzzling. Numerical simulations suggest that the MB formed...
  • Publication
    The Magellanic System: the puzzle of the leading gas stream
    The Magellanic Clouds (MCs) are the most massive gas-bearing systems falling into the Galaxy at the present epoch. They show clear signs of interaction...
  • Publication
    The MAGIC Telescope and the observation of Gamma Ray Bursts
    The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able to take full advantage of the fast slewing capability of its...
  • Publication
    The magnetic canopy above light bridges
    An analysis of high-resolution Stokes observations of two light bridges in active region NOAA 8990 is presented. The observations were recorded with the La...
  • Publication
    The magnetic field configuration of a solar prominence inferred from spectropolarimetric observations in the He i 10 830 Å triplet
    Context. Determining the magnetic field vector in quiescent solar prominences is possible by interpreting the Hanle and Zeeman effects in spectral lines...
  • Publication
    The magnetic field of the AP star Epsilon UMa
    The magnetic field of the Ap star Epsilon UMa was measured using the Zeeman-Doppler Imaging method. Ultrahigh S/N polarized profiles of the 4923 A magnetically...