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)...
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...
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...
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...
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...
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...
Comparison of Bar Strengths in the Optical and Near-infrared
Bars are expected to play an important role in galactic dynamics. Since the rest-frame wavelength of near-infrared images of high redshift galaxies lies in the...