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researcher

C. Ng

3 papers hereh-index 8174 citations17 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
same name
  • C. Ng — 19 papers, h 32
  • C. Ng — 13 papers, h 12
  • C. Ng — 9 papers, h 39
  • C. Ng — 6 papers, h 17
  • C. Ng — 3 papers, h 51
  • C. Ng — 2 papers, h 22

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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

39 citations · 67 across the 2 of their papers we have counts for

collaborators

3 papers

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★ 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…

astro-ph.HE2016

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.