Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...2e..13k&link_type=abstract
On the Present and Future of Pulsar Astronomy, 26th meeting of the IAU, Joint Discussion 2, 16-17 August, 2006, Prague, Czech Re
Astronomy and Astrophysics
Astronomy
Scientific paper
A simple analytical approximation of the form of low-energy cut-off of the secondary particle distribution is proposed. This approximation is acceptable for describing the known cascade numerical simulation [1]. The distribution form and maximum position as function of pulsar parameters have been found theoretically by considering the curvature radiation process and the electron-positron pairs production [2, 3]. An influence of synchrotron radiation [4] on the form and maximum of the low-energy distribution is considered. [1] Harding A. K., Daugherty J. K., ApJ, 252, 337, 1982. [2] Beskin V. S., Usp. Fiz. Nauk 169, 1169, 1999. [3] Malov I. F., Radiopulsars, Moscow, Nauka, 2004, 192 p. [4] Gurevich A. V., Isomin Ya. N., Zh. Eksp. Teor. Fiz. 89, 3, 1985.
Flanchik Alexander B.
Kontorovich Victor M.
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