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Browsing Publications of Astronomical Society of India by Author "Kapoor, R. C"

Browsing Publications of Astronomical Society of India by Author "Kapoor, R. C"

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  • Kapoor, R. C; Shukre, C. S (Astronomical Society of India, 2001)
    Pulsar radio pulses are made up of the so called core and conal components. A remarkably precise relation for core component widths, found observationally, in effect specifies the size of the polar cap on pulsars. Inclusion ...
  • Kapoor, R. C (Astronomical Society of India, 1976-03)
  • Kapoor, R. C (Astronomical Society of India, 1986-09)
    The astrophysical aspects of proposals of escape of supermassive blackholes from galactic nuclei and their implications in relation to quasars are discussed. We conclude that high velocity recoil of the central engine can ...
  • Datta, B; Kapoor, R. C (Astronomical Society of India, 1984-12)
    General relativistic effects of rotation on the structure and surface emission of the fast pulsar PSR 1937 + 214 are illustrated using a rotationally perturbed interior spherical metric. The results are found to differ ...
  • Kapoor, R. C; Shukre, C. S (Astronomical Society of India, 1999)
  • Kapoor, R. C (Astronomical Society of India, 1981-09)
    An analytical study has been carried out of the non-tangential emission of photons in the orbital plane from a monochromatic source of radiation orbiting a blackhole, using the method of geometrical optics. The formulation ...
  • Kapoor, R. C (Astronomical Society of India, 1976-12)
  • Kapoor, R. C; Shukre, C. S (Astronomical Society of India, 2002-09)
    By attributing the often seen longitude offsets between the core and conal component centres of pulsar radio pulses to different emission altitudes, we present a new method for investigating these altitudes. OUf method ...
  • Datta, B; Kapoor, R. C (Astronomical Society of India, 1985-09)
    Propagation of photons in the spacetime exterior to a rapidly rotating neutron star is investigated, using a rotationally perturbed spherical metric, to determine the pulse profile of fast pulsars. We find that spacetime ...

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