Astrophysical: Magellanic Clouds

  • Publication
    Toward an Internally Consistent Astronomical Distance Scale
    Accurate astronomical distance determination is crucial for all fields in astrophysics, from Galactic to cosmological scales. Despite, or perhaps because of...
  • Publication
    Two newly identified, relatively old star clusters in the Small Magellanic Cloud
    We present the results on the age and metallicity estimates of the Small Magellanic Cloud (SMC) clusters L110, L112 and L113 obtained from CCD Washington CT1...
  • Talk
    Unveiling the evolutionary history of the Magellanic Clouds through detection and analysis of stellar over-densities: clusters and streams.
    The Magellanic Clouds (MCs) are the closest example of a three-body interacting system composed of the Milky Way (MW), the Large Magellanic Cloud (LMC), and the...
  • Publication
    VLT-FLAMES survey of massive stars (Hunter+, 2008)
    As part of a European Southern Observatory (ESO) Large Programme on the Very Large Telescope (VLT, Paranal, Chile) observations were obtained for over 700 stars...
  • Publication
    VLT-FLAMES Tarantula Survey (Evans+, 2011)
    The Tarantula Survey employs three modes of the Fibre Large Array Multi-Element Spectrograph (FLAMES) instrument on the VLT: Medusa-Giraffe, ARGUS-Giraffe and...
  • Publication
    X-Shooting ULLYSES: Massive stars at low metallicity. II. DR1: Advanced optical data products for the Magellanic Clouds
    Context. The XShootU project aims to obtain ground-based optical to near-infrared spectroscopy of all targets observed by the Hubble Space Telescope (HST) under...
  • Publication
    X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars
    Context. The winds of massive stars have a significant impact on stellar evolution and on the surrounding medium. The maximum speed reached by these outflows...