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Geodetic Precession in PSR B1534+12

  • Stairs I
  • Thorsett S
  • Taylor J
  • et al.
International Astronomical Union Colloquium (2000) 177 121-124
DOI: 10.1017/s0252921100059224
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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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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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