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Predictions of inverse Compton radiation from PSR B1259–63

Published online by Cambridge University Press:  12 April 2016

J. G. Kirk ,
Lewis Ball  and
O. Skjæraasen
J. G. Kirk
Affiliation:
Max-Planck-Institut für Kernphysik, Postfach 10 39 80, D-69029, Heidelberg, Germany
Lewis Ball
Affiliation:
Research Centre for Theoretical Astrophysics, University of Sydney, N.S. W. 2006, Australia
O. Skjæraasen
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway

Extract

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Unpulsed high energy (TeV) emission has been detected from several isolated pulsars (Aharonian 1999) and presumably results from relativistic electrons accelerated at the termination shock of an MHD wind driven by the pulsar itself. These electrons inverse Compton scatter target photons from either the cosmic microwave background, or from their own synchrotron radiation.

The rotation-powered binary pulsar PSR B1259–63 (Johnston et al. 1996) is also thought to drive an MHD wind, and the synchrotron radiation of electrons accelerated at its termination shock is probably the source of the unpulsed X-rays seen from this object by ROSAT, OSSE and ASCA (Tavani & Arons 1997). Compared to the isolated pulsars, however, the the pulsar’s Be-star companion provides an energy density of target photons available for inverse Compton scattering which is some 11 orders of magnitude larger. Using delta-function approximations to the emissivities and a monochromatic approximation to the spectrum of the target photons, we modelled the observed X-ray synchrotron emission and predicted the TeV emission in a recent paper (Kirk et al. 1999). In this contribution we improve these calculations in two respects – by treating the target spectrum more precisely, as described in the companion paper (Ball & Kirk 1999), and by relaxing the approximations made in the emissivities.

Type
Part 7. The Surrounding of Pulsars
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 531 - 532
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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Johnston, S., et al., 1996, MNRAS, 279, 1026 CrossRefGoogle Scholar
Kirk, J.G., Ball, L., Skjæraasen, O., 1999, Astroparticle Phys., 10, 31 CrossRefGoogle Scholar
Matsubara, Y. 1997 in proceedings of “Towards a Major Atmospheric Cherenkov Detector V”, Kruger National Park, Ed: de Jager, O.C., p. 447 Google Scholar
Tavani, M., Arons, J., 1997, ApJ, 477, 439 Google Scholar