Publication type: Non-refereed

  • Publication
    On the classification of ultra-compact nuclear rings
    Ultra-compact nuclear rings (UCNRs) can be defined as those galactic circumnuclear rings with a radius inferior to 200 parsecs [1]. Because very high spatial...
  • Publication
    On the colors of barlenses and their link to B/P bulges
    Barlenses are morphological features present in barred galaxies with morphological types between S0 and Sb. Recently, they have been suggested to be the more...
  • Publication
    On the continuum intensity-magnetic field relation along the decay phase of sunspots
    A continuum intensity-magnetic field distributions are presented for a decaying sunspot. It is shown that a very simple model accounts for the observed...
  • Publication
    On The Cooling Tails Of Thermonuclear X-ray Bursts: News From Terzan 5
    The neutron star transient and 11 Hz X-ray pulsar IGR J17480-2446, recently discovered in the globular cluster Terzan 5, showed unprecedented bursting activity...
  • Publication
    On The Cooling Tails Of Thermonuclear X-ray Bursts: News From Terzan 5
    The neutron star transient and 11 Hz X-ray pulsar IGR J17480-2446, recently discovered in the globular cluster Terzan 5, showed unprecedented bursting activity...
  • Publication
    On the curvature of dust lanes in galactic bars
    Not Available
  • Publication
    On the Dependence of our Inferences about the Solar Internal Rotation on the Frequency Fitting Methodology
    We show how inferences of the solar internal rotation rate depend on different aspects of the mode fitting procedure. We study the stability of the rotation...
  • Publication
    On the Detectability of Post-common-envelope Binary Central Stars of Planetary Nebulae
    Common envelope evolution is widely accepted as the principal shaping agent in the formation of aspherical planetary nebulae. However, only some 20% of...
  • Publication
    On the Determination of Magnetic Field Strength and Flux in Inter-Network
    The results of the determination of magnetic field strength and flux from weak polarimetric signals in solar inter-network regions are contradictory. We...