Publicaciones

  • FCC-hh: The Hadron Collider. Future Circular Collider Conceptual Design Report Volume 3

    In response to the 2013 Update of the European Strategy for Particle Physics (EPPSU), the Future Circular Collider (FCC) study was launched as a world-wide international collaboration hosted by CERN. The FCC study covered an energy-frontier hadron collider (FCC-hh), a highest-luminosity high-energy lepton collider (FCC-ee), the corresponding 100 km

    Abada, A. et al.

    Fecha de publicación:

    7
    2019
  • Spectral energy distributions and luminosities of M dwarfs in the CARMENES search for exoplanets

    In the quest for Earth-sized exoplanets, M dwarfs are stars of increasing interest during the last two decades. Their small sizes and masses as compared to our Sun make them specially suitable targets to look for the signatures of planetary companions, as their habitable zones fall closer to their host star. Despite being the most abundant stars in

    Cifuentes, C. et al.

    Fecha de publicación:

    3
    2019
  • Mixed properties of MHD waves in non-uniform plasmas

    This paper investigates the mixed properties of MHD waves in a non-uniform plasma. It starts with a short revision of MHD waves in a uniform plasma of infinite extent. In that case the MHD waves do not have mixed properties. They can be separated in Alfvén waves and magneto-sonic waves. The Alfvén waves propagate parallel vorticity and are

    Goossens, Marcel L. et al.

    Fecha de publicación:

    4
    2019
  • Influence of magnetic activity on the determination of stellar parameters through asteroseismology

    Magnetic activity changes the gravito-acoustic modes of solar-like stars and in particular their frequencies. There is an angular-degree dependence that is believed to be caused by the non-spherical nature of the magnetic activity in the stellar convective envelope. These changes in the mode frequencies could modify the small separation of low

    Pérez Hernández, Fernando et al.

    Fecha de publicación:

    5
    2019
  • Fornax 3D project: a two-dimensional view of the stellar initial mass function in the massive lenticular galaxy FCC 167

    The stellar initial mass function (IMF) regulates the baryonic cycle within galaxies, and is a key ingredient for translating observations into physical quantities. Although it was assumed to be universal for decades, there is now growing observational evidence showing that the center of massive early-type galaxies hosts a larger population of low

    Martín-Navarro, I. et al.

    Fecha de publicación:

    6
    2019