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C. Nixon

24 papers hereh-index 9342 citations15 works total

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

author position
  • first author7
  • middle author6
  • last author9

Across the 22 of 24 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE19
  • astro-ph.EP2
  • astro-ph.GA2
  • astro-ph.SR1
same name
  • C. Nixon — 63 papers, h 30
  • C. Nixon — 28 papers, h 42
  • C. Nixon — 17 papers, h 13
  • C. Nixon — 12 papers, h 4
  • C. Nixon — 9 papers, h 4
  • C. Nixon — 7 papers, h 3

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
20182026
most citedDisc tearing: implications for black hole accretion and AGN variability

100 citations · 597 across the 24 of their papers we have counts for

collaborators
Showing 2018Show all

4 papers · 1 filter

astro-ph.HE2018★ 15 cited

An ultra-fast inflow in the luminous Seyfert PG1211+143

Ken Pounds, Chris Nixon, Andrew Lobban +1

Blueshifted absorption lines in the X-ray spectra of AGN show that ultra-fast outflows with typical velocities v∼0.1c are a common feature of these luminous objects. Such po…

astro-ph.GA2018★ 4 cited

Does slow and steady win the race? Investigating feedback processes in giant molecular clouds

L. Garratt-Smithson, G. A. Wynn, C. Power +1

We investigate the effects of gradual heating on the evolution of turbulent molecular clouds of mass 2×106 M⊙​ and virial parameters ranging between 0.7−1.2. This…

astro-ph.EP2018★ 31 cited

The Maximum Mass Solar Nebula and the early formation of planets

C. J. Nixon, A. R. King, J. E. Pringle

Current planet formation theories provide successful frameworks with which to interpret the array of new observational data in this field. However, each of the two main theories (c…

astro-ph.HE2018★ 45 cited

Instability of warped discs

S. Doğan, C. J. Nixon, A. R. King +1

Accretion discs are generally warped. If a warp in a disc is too large, the disc can `break' apart into two or more distinct planes, with only tenuous connections between them. Fur…

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