39 citations · 179 across the 9 of their papers we have counts for
9 papers
The X-ray modulation of PSR J2032+4127/MT91 213 during the Periastron Passage in 2017
K. L. Li, J. Takata, C. W. Ng +4
We present the Neil Gehrels Swift Observatory (Swift), Fermi Large Area Telescope (Fermi-LAT), and Karl G. Jansky Very Large Array (VLA) observations of the gamma-ray binary PSR J2…
Mode change of a gamma-ray pulsar, PSR J2021+4026
J. Zhao, C. W. Ng, L. C. C. Lin +8
A glitch of a pulsar is known as a sudden increase in the spin frequency and spin-down rate (frequency time derivative), and it can be caused by a sudden rel\ ease of the stress bu…
Modeling the High-energy Emission from the Gamma-ray Binary 1FGL J1018.6-5856
A. M. Chen, C. W. Ng, J. Takata +1
1FGL J1018.6-5856 is a high mass gamma-ray binary containing a compact object orbiting around a massive star with a period of 16.544 d. If the compact object is a pulsar, non-therm…
High-Energy emissions from the Pulsar/Be binary system PSR J2032+4127/MT91 213
J. Takata, P. H. T. Tam, C. W. Ng +4
PSR J2032+4127 is a radio-loud gamma-ray-emitting pulsar; it is orbiting around a high-mass Be type star with a very long orbital period of 25-50years, and is approaching periastro…
Differences between radio-loud and radio-quiet gamma-ray pulsars as revealed by Fermi
C. Y. Hui, Jongsu Lee, J. Takata +2
By comparing the properties of non-recycled radio-loud ray pulsars and radio-quiet ray pulsars, we have searched for the differences between these two populations. We found…
Observation and Simulation of the Variable Gamma-ray Emission from PSR~J2021+4026
C. W. Ng, J. Takata, K. S. Cheng
Pulsars are rapidly spinning and highly magnetized neutron stars, with highly stable rotational period and gradual spin-down over a long timescale due to the loss of radiation. Gli…