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The microlensing probability of the pulsars located in globular clusters

Published online by Cambridge University Press:  12 April 2016

Tanya Larchenkova
Tanya Larchenkova*
Affiliation:
Astro Space Center of P.N.Lebedcv Physical Institute, Profsoyuznaya 84/32, Moscow 117810RUSSIA

Abstract

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We have used the effect of Shapiro delay of the pulsar radiation in the gravitational lensing approximation. The microlensing probabilities for pulsars located in globular clusters 47 Tuc (NGC 104) and M15 (7078) in the case of rather large impact parameters was calculated.

Type
Part 2. Timing, General Relativity and Astrometry
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 89 - 90
Copyright
Copyright © Astronomical Society of the Pacific 2000

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