Publication type: Non-refereed

  • Publication
    Compact Groups of Galaxies: Evolution of the Stellar Population
    We present a study focusing on the nature of compact groups (CGs) through the study of their elliptical (E) galaxies. Parameters describing the internal...
  • Publication
    Compact radio emission in Ultraluminous X-ray sources
    Not Available
  • Publication
    Compact radio emission in Ultraluminous X-ray sources
    We present results from our studies of radio emission from selected Ultraluminous X-ray (ULX) sources, using archival Giant Metrewave Radio Telescope (GMRT)...
  • Publication
    Compact radio-loud Broad Absorption Line Quasars .
    For a long time, radio-loud Broad Absorption Line Quasars (BAL QSOs) were thought to be extremely rare objects. The absorbing troughs seen in their optical...
  • Publication
    Comparing Absolute Near-UV Fluxes of Late-Type Stars with the Predictions of Model Atmospheres (CD-ROM Directory: contribs/allende1)
    Not Available
  • Publication
    Comparing peanut-shaped `bulges' to N-body simulations and orbital calculations
    We present a near-infrared K n-band photometric study of edge-on galaxies with a box/ peanut-shaped `bulge'. The morphology of the galaxies is analysed using...
  • Publication
    Comparing polarized submm emission and near-infrared extinction polarization in the Vela C giant molecular cloud
    We present one of largest studies to date of combined near-infrared and submillimeter linear polarization data for a giant molecular cloud. The dust polarized...
  • Publication
    Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud
    We present a large-scale combination of near-infrared (near-IR) interstellar polarization data from background starlight, with polarized emission data at sub...
  • Publication
    Comparing the Observed Frequencies of Balloon 09010001 with Theoretical Modes of Oscillation
    Balloon 090100001 has turned out to be one of the most interesting pulsating sdB stars. However, its interest compares with the difficulty for it to be modelled...