Geodetic Precession in PSR B1534+12

I. H. Stairs; J. H. Taylor; S. E. Thorsett; Z. Arzoumanian

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Geodetic Precession in PSR B1534+12

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arxiv astro-ph/9911198 v2 pith:MBEZONZI submitted 1999-11-11 astro-ph

I. H. Stairs , S. E. Thorsett , J. H. Taylor , Z. Arzoumanian This is my paper · ORCID

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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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