Geodetic Precession in PSR B1534+12

Details Geodetic Precession in PSR B1534+12 Geodetic Precession in PSR B1534+12

1999-11-11

arxiv.org/abs/astro-ph/9911198v2

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures. Corrected a reference. To appear in proceedings of IAU Colloquium 177: Pulsar Astronomy - 2000 and Beyond

Scientific paper

We present Arecibo observations of PSR B1534+12 which confirm previous
suggestions that the pulse profile is evolving secularly. This effect is
similar to that seen in PSR B1913+16, and is almost certainly due to general
relativistic precession of the pulsar's spin axis.

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