Long Term Timing Observations of PSR B1509-58

Details Long Term Timing Observations of PSR B1509-58 Long Term Timing Observations of PSR B1509-58

2004-02-08

arxiv.org/abs/astro-ph/0402181v1

Astronomy and Astrophysics

Astrophysics

2 pages. To appear in "Young Neutron Stars and Their Environments"(IAU Symposium 218, ASP Conference Proceedings), eds F. Cami

Scientific paper

We present an updated phase-coherent timing solution for the young, energetic
pulsar PSR B1509-58 for twenty years of data. Using a partially phase-coherent
timing analysis, we show that the second frequency derivative is changing in
time implying a third frequency derivative of (-9+/-1)x10^-32 s^(-4). This
value is consistent with the simple power law model of pulsar rotation.

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