Tipo de publicación: Con árbitro

  • Publicación
    Constraining the Evolution of ZZ Ceti
    We report our analysis of the stability of pulsation periods in the DAV star (pulsating hydrogen atmosphere white dwarf) ZZ Ceti, also called R 548. Based on...
  • Publicación
    Constraining the Evolution of ZZ Ceti
    We report our analysis of the stability of pulsation periods in the DAV star (pulsating hydrogen atmosphere white dwarf) ZZ Ceti, also called R548. On the basis...
  • Publicación
    Constraining the formation of inner bars: photometry, kinematics and stellar populations in NGC 357
    Double-barred galaxies are common in the local Universe, with approximately one-third of barred spirals hosting a smaller, inner bar. Nested bars have been...
  • Publicación
    Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
    We present a method to produce mock galaxy catalogues with efficient perturbation theory schemes, which match the number density, power spectra and bispectra in...
  • Publicación
    Constraining the inner density slope of massive galaxy clusters
    We determine the inner density profiles of massive galaxy clusters (M 200 > 5 × 10 14 M ☉) in the Cluster-EAGLE (C-EAGLE) hydrodynamic simulations, and...
  • Publicación
    Constraining the magnetic vector in the quiet solar photosphere and the impact of instrumental degradation
    Context. With the advent of next generation high resolution telescopes, our understanding of how the magnetic field is organized in the internetwork (IN)...
  • Publicación
    Constraining the nature of high frequency peakers. II. Polarization properties
    Aims:The “bright” High Frequency Peakers (HFPs) sample is a mixture of blazars and intrinsically small and young radio sources. We investigate the polarimetric...
  • Publicación
    Constraining the nature of the accreting binary in CXOGBS J174623.5-310550
    We report optical and infrared observations of the X-ray source CXOGBS J174623.5-310550. This Galactic object was identified as a potential quiescent low-mass X...
  • Publicación
    Constraining the oblateness of transiting planets with photometry and spectroscopy
    Rapid planetary rotation can cause the equilibrium shape of a planet to be oblate. While planetary oblateness has mostly been probed by examining the subtle...