Weak microlensing effect and stability of pulsar time scale
Astrophysics
2007-05-23 v1
Abstract
An influence of the weak microlensing effect on the pulsar timing is investigated for pulsar B1937+21. Average residuals of Time of Arrival (TOA) due to the effect would be as large as 10 ns in 20 years observation span. These residuals can be much greater (up to 1 ms in 20 years span) if pulsar is located in globular cluster (or behind it).
Keywords
Cite
@article{arxiv.astro-ph/0610681,
title = {Weak microlensing effect and stability of pulsar time scale},
author = {M. S. Pshirkov and M. V. Sazhin},
journal= {arXiv preprint arXiv:astro-ph/0610681},
year = {2007}
}
Comments
11 pages, 7 figures