Tipo de publicación: Sin árbitro

  • Publicación
    On the radial distribution of white dwarfs in the Galactic globular cluster omega Cen
    We present deep and accurate photometry (F435W, F625W, F658N) of the Galactic Globular Cluster omega Cen collected with the Advanced Camera for Surveys (ACS) on...
  • Publicación
    On the Radial Velocity Distribution of the Carina dSph galaxy
    We present the radial velocity (RV) distribution of Carina dSph, obtained using low-, medium- and high-resolution spectroscopic data collected with FORS2 and...
  • Publicación
    On the Relation between Radio and Non-Radio Elliptical Galaxies
    Empirical evidence suggests that elliptical galaxies hosting a radio source may not be different from normal non-radio ellipticals. To test this possibility, we...
  • Publicación
    On the relation between the maximum stellar mass and the star cluster mass.
    Not Available
  • Publicación
    On the relation of the Duvall phase function to the upper layers on the convection zone
    A method to obtain the Duvall phase function from the structure of a stellar model is presented. This can be a good tool for understanding the dependence of p...
  • Publicación
    On the relations between X-ray binaries and binary pulsars
    Not Available
  • Publicación
    On the relationship between dynamical masses from spectral features in emission and other mass estimators for a sample of local star-forming galaxies
    We have obtained both virial and dynamical masses of a sample oflocal star forming galaxies from the UCM survey. The rotational curvesmeasured using the...
  • Publicación
    On the Relationship between Star Formation and Activity in Galaxies
    This thesis is made of three main parts. In the first one a sample of 55 galaxies with an active nucleus (Seyfert 1, Seyfert2 and LINERs) is analysed; these...
  • Publicación
    On the sensitivity of the Halpha scattering polarization to chromospheric magnetism
    A particularly interesting line for exploring the physical conditions of the quiet solar chromosphere is Halpha , but its intensity profile is magnetically...