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Long-term Radio Timing Observations of PSR B1509–58
Published online by Cambridge University Press: 19 July 2016
Abstract
We present an updated phase-coherent timing solution for the young, energetic pulsar B1509–58 from 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 This value is consistent with the simple power law model of pulsar rotation.
- Type
- Part 10: Radio Pulsar Timing
- Information
- Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 425 - 426
- Copyright
- Copyright © Astronomical Society of the Pacific 2004