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19942007
most citedInfluence of the jet opening angle on the derived kinematical parameters of blazar jets having uniform and stratified bulk motion

15 citations · 19 across the 7 of their papers we have counts for

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astro-ph200715 cited

Influence of the jet opening angle on the derived kinematical parameters of blazar jets having uniform and stratified bulk motion

Gopal-Krishna, Samir Dhurde, Pronoy Sircar +1

We present analytical modelling of conical relativistic jets, in order to evaluate the role of the jet opening angle on certain key parameters that are inferred from VLBI radio obs…

astro-ph2007

Effects of Jet Opening Angle and Velocity Structure on Blazar Parameters

Paul J. Wiita, Gopal-Krishna, Samir Dhurde +1

We had earlier shown that for a constant velocity jet the discrepancy between the low speeds indicated by VLBI knot motions and the high Doppler factors inferred from emission of T…

astro-ph2007

Further evidence for intra-night optical variability of radio-quiet quasars

A. Goyal, Gopal-Krishna, Ram Sagar +2

Although well established for BL Lac objects and radio-loud quasars, the occurrence of intra-night optical variability (INOV) in radio-quiet quasars is still debated, primarily sin…

astro-ph2004

Expansion of radio galaxies in a cosmologically evolving medium: Possible implications for the cosmic star-formation history

Paramita Barai, Gopal-Krishna, M. Angela Osterman +1

We compare earlier estimates of the volumes filled by lobes of radio galaxies during the quasar era based upon non-evolving ambient media with new ones assuming a strong cosmologic…

astro-ph20044 cited

Asymmetries in Powerful Extragalactic Radio Sources

Gopal-Krishna, Paul J. Wiita

This review provides the background and current perspective of some of the striking asymmetries exhibited by extragalactic double-lobed radio sources, paying special attention to t…

astro-ph2003

Radio Galaxies and the Magnetization of the IGM

Gopal-Krishna, Paul J. Wiita

Observed radio galaxies had a much higher comoving density during the `quasar era', at z ~ 2-3, but these sources are only detectable for small fractions of their active lifetimes…