M
M. Coleman Miller
Researcher at University of Maryland, College Park
Publications - 305
Citations - 14363
M. Coleman Miller is an academic researcher from University of Maryland, College Park. The author has contributed to research in topics: Neutron star & Black hole. The author has an hindex of 68, co-authored 293 publications receiving 12880 citations. Previous affiliations of M. Coleman Miller include University of Copenhagen & Johns Hopkins University.
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Journal ArticleDOI
A unified model for tidal disruption events
Lixin Dai,Lixin Dai,Jonathan C. McKinney,Nathaniel Roth,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,M. Coleman Miller +6 more
TL;DR: In this paper, the super-Eddington compact disk phase of TDEs has been studied using three-dimensional general relativistic radiation magnetohydrodynamics simulations.
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Super-Eddington fluxes during thermonuclear X-ray bursts
TL;DR: In this paper, it was shown that the Bose-Einstein spectra of the Rossi X-ray Timing Explorer (SXT) measurements of the 4U 1820-30 superburst and a long burst from GX 17+2 are well-fit by similar BoseEinstein Spectra with high temperatures and modest chemical potentials.
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Phase lags in Cygnus X-1
TL;DR: In this article, it was shown that the functional dependence of lag on Fourier frequency emerges intact from transit through the corona, modulo a multiplicative factor (which may in principle be negative, so that a phase lag can be changed to a phase lead).
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Energetic constraints on electromagnetic signals from double black hole mergers
Lixin Dai,Lixin Dai,Jonathan C. McKinney,Jonathan C. McKinney,M. Coleman Miller,M. Coleman Miller +5 more
TL;DR: In this article, it was shown that the heat produced by the dynamical friction on such black hole orbits can exceed the stellar binding energy by a large factor, which means that this heat could destroy the star and thus make it difficult for enough gas to be near the holes at merger to produce detectable photons.
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A characterization of the brightness oscillations during thermonuclear bursts from 4u 1636(536
TL;DR: In this article, the authors analyzed the brightness oscillations in the initial 0.75 s of the five bursts that were used in a previous search for a brightness oscillation at the expected ~290 Hz spin frequency.