39 citations · 179 across the 9 of their papers we have counts for
Showing 2017Show all
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astro-ph.HE2017★ 28 cited
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…
astro-ph.HE2017★ 3 cited
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…
astro-ph.HE2017★ 39 cited
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…