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19942013
most citedReconnection in a striped pulsar wind

403 citations · 1.9k across the 20 of their papers we have counts for

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17 papers · 1 filter

astro-ph2007★ 11 cited

A synchrotron self-Compton model with low energy electron cut-off for the blazar S5 0716+714

Olivia Tsang, J. G. Kirk

Rapid inverse Compton cooling sets in when the brightness temperature (T_B) of a self-absorbed synchrotron source with power-law electrons reaches ~10^{12} K. However, T_B inferred…

astro-ph2006★ 19 cited

The inverse Compton catastrophe and high brightness temperature radio sources

Olivia Tsang, J. G. Kirk

The occurrence of the inverse Compton catastrophe when the synchrotron brightness temperature exceeds a threshold value, usually estimated to be 10^{12} K, appears to be in contrad…

astro-ph2005★ 1 cited

The high-energy gamma-ray light curve of PSR B1259 -63

J. G. Kirk, Lewis Ball, S. Johnston

The high-energy gamma-ray light curve of the binary system PSR B1259 -63, is computed using the approach that successfully predicted the spectrum at periastron. The simultaneous IN…

astro-ph2005★ 91 cited

Polarization of high-energy pulsar radiation in the striped wind model

J. Petri, J. Kirk

The Stokes parameters of the pulsed synchrotron radiation produced in the striped pulsar wind model are computed and compared with optical observations of the Crab pulsar. We assum…

astro-ph2005★ 2 cited

Dissipation in Pulsar Winds

J. G. Kirk

I review the constraints placed on relativistic pulsar winds by comparing optical and X-ray images of the inner Crab Nebula on the one hand with two-dimensional MHD simulations on…

astro-ph2003★ 139 cited

Modelling the TeV gamma-ray spectra of two low redshift AGNs: Mkn 501 and Mkn 421

Alexander K. Konopelko, Apostolos Mastichiadis, John G. Kirk +2

We discuss the results of modelling the TeV gamma-ray spectra of two AGNs, Mkn 501 and Mkn 421 that have almost the same redshifts: z=0.031 and z=0.034, respectively. The effect of…