Abstract
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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CITATION STYLE
APA
Stairs, I. H., Thorsett, S. E., Taylor, J. H., & Arzoumanian, Z. (2000). Geodetic Precession in PSR B1534+12. International Astronomical Union Colloquium, 177, 121–124. https://doi.org/10.1017/s0252921100059224
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