ForumSpringerAstron. Astrophys.
ForumWhats NewSearchOrders

Astron. Astrophys. 317, 99-103 (1997)

Table of Contents
Available formats: HTML | PDF (159 KB) | (gzipped) PostScript (240 KB)

The TeV [FORMULA] -ray visibility of Geminga-like pulsars

R.K. Kaul

Bhabha Atomic Research Centre, Nuclear Research Laboratory, Trombay, Bombay - 400 085, India

Received 17 August 1995 / Accepted 17 May 1996


It is shown that, while the number of Geminga-like pulsars in the Galaxy may be [FORMULA], the prospects of detecting TeV gamma-ray signals from them are not very encouraging. Arguments are presented to show that Geminga-like pulsars having periods in the range 200-500 ms, surface magnetic fields [FORMULA] Gauss and preferentially located within [FORMULA] of the earth may be able to produce detectable TeV gamma-ray signals.

Key words: pulsars: individual: Geminga — pulsars: general — gamma rays: theory

© European Southern Observatory (ESO) 1997