Publication type: Non-refereed

  • Publication
    Physical properties of 5 near-Earth asteroids observed with the Arecibo Planetary Radar within NEOROCKS project.
    The near-Earth object (NEO) population is composed of asteroids and comets that have orbits close to the Earth. This vicinity to the Earth gives us some...
  • Publication
    Physical properties of asteroids derived from a novel approach to modeling of optical lightcurves and WISE thermalinfrared data
    Convex shape models and spin vectors of asteroids are now routinely derived from their disk-integrated lightcurves by the lightcurve inversion method of...
  • Publication
    Physical Properties of Binary Brown Dwarfs
    Astrometric observations of binary brown dwarfs yield dynamical masses of the components independently of theoretical models. We give an update on our long-term...
  • Publication
    Physical properties of H alpha selected star forming galaxies at z = 0.84
    In this work we analyze the star formation rates and stellar masses of a sample of 157 star forming galaxies at z ˜ 0.84 (Villar et al. 2008), selected by their...
  • Publication
    Physical properties of Hi'iaka from stellar occultation data
    Two very bright stellar occultations by Hi'iaka, the largest satellite of the dwarf planet Haumea, were predicted to take place during in April 2021. Since the...
  • Publication
    Physical properties of NEOs derived from their phase curves
    IntroductionThe observation of NEOs allows us to study the physical characteristics of the smallest size bodies of our Solar System as well as to impose...
  • Publication
    Physical properties of the cubewano 19521 Chaos from a multi-chord stellar occultation
    Trans-Neptunian Objects (TNOs) have had an increasing interest since the discovery of (15760) Albion in 1992. These objects are considered remnants of the Solar...
  • Publication
    Physical requirements for modeling stellar atmospheres according to the different spectral features observed
    Not Available
  • Publication
    Physical Scenarios for Supersonic Gas Flows Observed in H II Regions
    Line profiles in ensuremath {{H}alpha } emission from H II region populations in spiral galaxies show emission features at +/-50 km/s from the main emission...