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The microlensing probability of the pulsars located in globular clusters
Published online by Cambridge University Press: 12 April 2016
Abstract
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