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Pulsar distance measurements using interstellar scintillation data

Published online by Cambridge University Press:  12 April 2016

T.V. Smirnova  and
V.I. Shishov
T.V. Smirnova
Affiliation:
Radio Astronomy Observatory of Astro Space Center, Lebedev Physical Institute, Pushchino, Moscow region 142292, Russia
V.I. Shishov
Affiliation:
Radio Astronomy Observatory of Astro Space Center, Lebedev Physical Institute, Pushchino, Moscow region 142292, Russia

Abstract

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We evaluate the distance to pulsars and the location of the effective scattering layer of turbulent medium along the line of sight on the base of analysis diffractive and refractive scintillation of pulsars. In some cases our estimations of distances to pulsars as more than 3 times differ from the values quoted in the TML pulsar catalog.

Type
Part 8. Pulsars and the Interstellar Medium
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 557 - 558
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Taylor, J.H., Manchester, R.N. &Lyne, A.G. 1993, ApJ, v. 88, p.529 Google Scholar
Stinebring, D.R. et al. 1996, Proc. in IAU Symp. 160, 455 Google Scholar
Smirnova, T.V., Shishov, V.I. &Stinebring, D.R. 1998, AZh, v. 42, p. 766 Google Scholar