Chandra Phase-resolved Spectroscopy of the High Magnetic Field Pulsar B1509-58
We report on a timing and spectral analysis of the young, high magnetic field rotation-powered pulsar (RPP) B1509-58 using Chandra continuous-clocking mode observation. The pulsar's X-ray light curve can be fit by the two Gaussian components and the pulsed fraction shows moderate energy depende...
| Main Authors: | , , , , |
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| Format: | Journal Article |
| Published: |
Institute of Physics Publishing
2017
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| Online Access: | http://hdl.handle.net/20.500.11937/52822 |