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Pulsar Interferometry with Microarcsecond Resolution

Published online by Cambridge University Press:  03 August 2017

A. Wolszczan  and
J. M. Cordes
A. Wolszczan
Affiliation:
NAIC, Arecibo Observatory, Arecibo, PR 00613
J. M. Cordes
Affiliation:
Astronomy Department and NAIC, Cornell University, Ithaca, NY 14853

Abstract

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An ‘interstellar interferometer’ related to a double imaging of the pulsar PSR 1237+25 by refraction in the interstellar medium has been used to resolve the pulsar magnetosphere for the first time. With an interferometer baseline ∼ 1 AU, we have measured a typical transverse separation between the emitting regions of PSR 1237+25 to be ∼ 108 cm, or an angular separation ∼ 0.02 μas.

Type
Galactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 285 - 286
Copyright
Copyright © Reidel 1988 

References

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