Discovery of Soft X-ray Pulsations from PSR J1231-1411 using NICER
arXiv:1905.12060 · doi:10.3847/2041-8213/ab2539
Abstract
We report the discovery of soft X-ray pulsations from the nearby millisecond pulsar PSR J12311411 using NICER. The pulsed emission is characterized by a broad and asymmetric main pulse and a much fainter secondary interpulse, with a total pulsed count rate of 0.055 c s in the 0.35-1.5 keV band. We analyzed Fermi LAT data to update the pulse timing model covering 10 years of data and used that model to coherently combine NICER data over a year of observations. Spectral modeling suggests that the flux is dominated by thermal emission from a hot spot (or spots) on the neutron star surface. The phase relationship between the X-ray pulse and the radio and rays provides insight into the geometry of the system.
ApJ Letters, in press
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Cited by in corpus (15)
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- Recycled pulsars with multipolar magnetospheres from accretion-induced magnetic burial
- Timing of Eight Binary Millisecond Pulsars Found with Arecibo in Fermi-LAT Unidentified Sources
- A Deep Chandra X-ray Observatory Study of the Millisecond Pulsar Population in the Globular Cluster Terzan 5
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- Phase resolved spectrum of the Crab pulsar from NICER
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- Bayesian Modeling of NICER Cometary X-ray Spectra: A Legacy Survey of Solar-Wind Charge Exchange