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A Search for Variable Interstellar Magnetic Fields and Neutron Star Precession in Four Years of Polarization Position Angle Measurements on 98 Pulsars
Published online by Cambridge University Press: 12 April 2016
Abstract
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We have studied the temporal behavior of linearly polarized position angle in a sample of 98 pulsars observed from Arecibo over a four–year period in a search for free precession and changes in interstellar magnetic fields along pulsar– earth lines of sight. We set upper limits on changes in position angle.
- Type
- Part 3. Studies of Radio Emission
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 269 - 270
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
Everett, J.E., & Weisberg, J.M.
1997, “The Free Precession of an Oblate Star,” Mathematica Notebook on the MathSource Library, at URL www.mathsource.com/cgi-bin/MathSource/Applications/Astronomy/0208-572
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Weisberg, J.M., Cordes, J.M., Lundgren, S.C., Dawson, B.R., Despotes, J.T., Morgan, J.J., Weitz, K.A., Zink, E.C., & Backer, D.C.
1999, ApJS, 121, 171
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