activity
20152017
most citedHigh-Energy emissions from the Pulsar/Be binary system PSR J2032+4127/MT91 213

39 citations · 171 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.HE20178 cited

Rapid X-ray variations of the Geminga pulsar wind nebula

C. Y. Hui, Jongsu Lee, A. K. H. Kong +4

A recent study by Posselt et al. (2017) reported the deepest X-ray investigation of the Geminga pulsar wind nebula (PWN) by using \emph{Chandra X-ray Observatory}. In comparison wi…

astro-ph.HE20177 cited

Searching for High Energy, Horizon-scale Emissions from Galactic Black Hole Transients during Quiescence

Lupin Chun-Che Lin, Hung-Yi Pu, Kouichi Hirotani +5

We search for the gamma-ray counterparts of stellar-mass black holes using long-term Fermi archive to investigate the electrostatic acceleration of electrons and positrons in the v…

astro-ph.HE201728 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.HE201719 cited

Lepton acceleration in the vicinity of the event horizon: Very-high-energy emissions from super-massive black holes

Kouichi Hirotani, Hung-Yi Pu, Lupin Chun-Che Lin +5

Around a rapidly rotating black hole (BH), when the plasma accretion rate is much less than the Eddington rate, the radiatively inefficient accretion flow (RIAF) cannot supply enou…

astro-ph.HE201729 cited

Swift, XMM-Newton, and NuSTAR observations of PSR J2032+4127/MT91 213

K. L. Li, A. K. H. Kong, P. H. T. Tam +3

We report our recent Swift, NuSTAR, and XMM-Newton X-ray and Lijiang optical observations on PSR J2032+4127/MT91 213, the gamma-ray binary candidate with a period of 45-50 years. T…

astro-ph.HE201715 cited

Search for GeV counterparts to fast radio bursts with Fermi

Shao-Qiang Xi, Pak-Hin Thomas Tam, Fang-Kun Peng +1

The non-repeating fast radio bursts (FRBs) could arise from catastrophic stellar explosions or magnetar giant flares, so relativistic blast waves might be produced in these events.…