Publication type: Non-refereed

  • Publication
    The Mirrors for the MAGIC Telescopes
    Not Available
  • Publication
    The missing mass conundrum of post-common-envelope planetary nebulae
    Most planetary nebulae (PNe) show beautiful, axisymmetric morphologies despite their progenitor stars being essentially spherical. Angular momentum provided by...
  • Publication
    The missing mass conundrum of post-common-envelope planetary nebulae
    Most planetary nebulae (PNe) show beautiful, axisymmetric morphologies despite their progenitor stars being essentially spherical. Angular momentum provided by...
  • Publication
    The MIUSCAT stellar population models: constraints from optical photometry
    We present the spectral extension of our stellar population synthesis models based on the MILES and CaT empirical stellar spectral libraries. For this purpose...
  • Publication
    The mixed Hodge structure on the fundamental group of hyperelliptic curves and higher cycles
    In this paper we give a geometrical interpretation of an extension of mixed Hodge structures (MHS) obtained from the canonical MHS on the group ring of the...
  • Publication
    The molecular diversity of TNOs revealed by JWST and its links to protoplanetary composition and processes
    Introduction: Bodies orbiting the trans-Neptunian regions (TNOs) are windows into Solar System formation, history and evolution. They are remnants from the...
  • Publication
    The molecular gas perspective on the growth and death of H emitters in the Spiderweb protocluster at Alpha z=2.16
    Galaxy clusters at low redshift are dominated by massive quiescent galaxies hosting stellar populations 10 Gyrs old, indicating that they were formed in the...
  • Publication
    The Mons campaign on OB stars
    In parallel with the monitoring of the periastron passage of the binary system WR 140, a number of B supergiants and Oe stars have been observed in the...
  • Publication
    The Morpho-kinematics of Planetary Nebulae with Binary Central Stars
    It is now clear that a binary formation pathway is responsible for a significant fraction of planetary nebulae, and this increased sample of known binaries...