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M. C. Miller

6 papers hereh-index 5243 citations6 works total

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

author position
  • middle author3
  • last author2

Across the 5 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.CO1
  • astro-ph.GA1
  • astro-ph.HE1
same name
  • M. C. Miller — 18 papers, h 9
  • M. C. Miller — 14 papers, h 6
  • M. C. Miller — 13 papers, h 8
  • M. C. Miller — 8 papers, h 3
  • M. C. Miller — 7 papers, h 16
  • M. C. Miller — 4 papers, h 6

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
20082010
most citedOn the time variability of geometrically-thin black hole accretion disks I : the search for modes in simulated disks

80 citations · 332 across the 6 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 74 cited

Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger

Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic +2

The association of an electromagnetic signal with the merger of a pair of supermassive black holes would have many important implications. For example, it would provide new informa…

astro-ph2008★ 42 cited

Origin of intermittent accretion-powered X-ray oscillations in neutron stars with millisecond spin periods

Frederick K. Lamb, Stratos Boutloukos, Sandor Van Wassenhove +3

We have shown previously that many of the properties of persistent accretion-powered millisecond pulsars can be understood if their X-ray emitting areas are near their spin axes an…

astro-ph2008★ 80 cited

On the time variability of geometrically-thin black hole accretion disks I : the search for modes in simulated disks

Christopher S. Reynolds, M. Coleman Miller

We present a detailed temporal analysis of a set of hydrodynamic and magnetohydrodynamic (MHD) simulations of geometrically-thin (h/r~0.05) black hole accretion disks. The black ho…

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