Publication type: Non-refereed

  • Publication
    Physical Conditions in the Partially Ionized Zone of the Orion Nebula
    We report the first reliable measurement of the nebular [O i] λ 5577 Angstroms emission line in the Orion nebula. Diagnostic diagrams based on the 5577 [O i]...
  • Publication
    Physical conditions of ionized gas and stellar populations in circumnuclear starbursts
    Not Available
  • Publication
    Physical parameters for the EXPORT sample. Rotational velocities and effective temperatures
    Not Available
  • Publication
    Physical parameters of low-ionization knots and jets in PNe: NGC 7009, K 4-47, and NGC 6543
    In addition to the large-scale outflows, which form their round, elliptical, and bipolar shells, planetary nebulae (PNe) also have, usually on smaller scales...
  • Publication
    Physical parameters of reflection nebulae in the galaxy
    Given observed equivalent widths of Mg II and Mg I absorptions due to an interstellar cloud in which a late-B star is embedded, it is shown that the basic...
  • Publication
    Physical parameters of the low-mass eclipsing binary NSVS 10653195
    NSVS 10653195 is a double-line detached eclipsing binary star found in 2007 by te{coughlin2007} among the NSVS periodic variable stars. The first analysis of...
  • Publication
    Physical parameters of V1430 Aql
    The aim of this study is to determine the physical parameters of the binary V1430 Aql from the study of light curves obtained in different filters V, R, I, J...
  • 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...