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C. Reynolds

33 papers hereh-index 7019.6k citations394 works total

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

author position
  • sole author2
  • first author8
  • middle author6
  • last author14

Across the 30 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph31
  • astro-ph.GA1
  • astro-ph.HE1
same name
  • C. Reynolds — 6 papers, h 23
  • C. Reynolds — 5 papers, h 18
  • C. Reynolds — 1 paper, h 2
  • C. Reynolds — 1 paper, h 14
  • C. Reynolds — 1 paper, h 1
  • C. Reynolds — 1 paper, h 5

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
19982009
most citedConstraining Black Hole Spin Via X-ray Spectroscopy

534 citations · 1.6k across the 16 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005

XMM-Newton Archival Study of the ULX Population in Nearby Galaxies

L. M. Winter, R. F. Mushotzky, C. S. Reynolds

We present the results of an archival XMM-Newton study of the bright X-ray point sources (L_X > 10^38 erg/s) in 32 nearby galaxies. From our list of approximately 100 point sources…

astro-ph2005

Oxygen and Iron Abundances in Nearby Galaxies Using Ultraluminous X-ray Sources

Lisa M. Winter, Richard F. Mushotzky, Christopher S. Reynolds

We determined oxygen and iron abundances of the interstellar medium (ISM) using K-shell (O) and L-shell (Fe) X-ray photo-ionization edges towards Ultra luminous X-ray sources (ULXs…

astro-ph2005

AGN Feedback and Cooling Flows: Problems with Simple Hydrodynamical Models

John C. Vernaleo, Christopher S. Reynolds

In recent years it has become increasingly clear that Active Galactic Nuclei, and radio-galaxies in particular, have an impact on large scale structure and galaxy formation. In pri…

astro-ph2005

Sporadically Torqued Accretion Disks Around Black Holes

David Garofalo, Christopher S. Reynolds

The assumption that black hole accretion disks possess an untorqued inner boundary, the so-called zero torque boundary condition, has been employed by models of black hole disks fo…

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