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researcher

C. Ng

3 papers hereh-index 3278 citations6 works total

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph.HE2
  • astro-ph1
same name
  • C. Ng — 153 papers, h 51
  • C. Ng — 104 papers, h 39
  • C. Ng — 87 papers, h 32
  • C. Ng — 42 papers, h 13
  • C. Ng — 40 papers, h 12
  • C. Ng — 23 papers, h 12

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

activity
19982023
most citedThe conductivity of dense molecular gas

230 citations · 269 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2023★ 14 cited

New constraints on the kinematic, relativistic and evolutionary properties of the PSR J1757−1854 double neutron star system

A. D. Cameron, M. Bailes, D. J. Champion +9

PSR J1757−1854 is one of the most relativistic double neutron star binary systems known in our Galaxy, with an orbital period of Pb​=4.4hr and an orbital eccent…

astro-ph.HE2022★ 25 cited

The High Time Resolution Universe Pulsar Survey -- XVII. PSR J1325-6253, a low eccentricity double neutron star system from an ultra-stripped supernova

R. Sengar, V. Balakrishnan, S. Stevenson +20

The observable population of double neutron star (DNS) systems in the Milky Way allow us to understand the nature of supernovae and binary stellar evolution. Until now, all DNS sys…

astro-ph1998★ 230 cited

The conductivity of dense molecular gas

Mark Wardle, Cindy Ng

We evaluate the conductivity tensor for molecular gas at densities ranging from 10^4 to 10^15 cm^-3 for a variety of grain models. The Hall contribution to the conductivity has gen…

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