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.
Papers
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Sonic-Point Model of Kilohertz Quasi-periodic Brightness Oscillations in Low-Mass X-Ray Binaries
TL;DR: In this paper, the authors proposed a model for the X-ray emission from 14 neutron stars in low-mass binary systems and from another neutron star in the direction of the Galactic center.
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Production of intermediate-mass black holes in globular clusters
TL;DR: In this paper, the authors explore a model for these sources and suggest that in some tens of per cent of globular clusters a very massive black hole, M≳50 m⊙, is formed.
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Intermediate - mass black holes
M. Coleman Miller,Edward Colbert +1 more
TL;DR: In the last few years, it was generally believed that black holes in nature appear in two broad mass ranges: stellar-mass (M ∼ 3 − 20 M⊙) which are produced by the core collapse of massive stars, and supermassive (m ∼ 10 6 − 10 10 10 M ⊙), which are found in the centers of galaxies and are generated by a still uncertain combination of processes as mentioned in this paper.
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Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA
Pau Amaro-Seoane,Jonathan R. Gair,Marc Freitag,M. Coleman Miller,Ilya Mandel,Curt Cutler,Stanislav Babak +6 more
TL;DR: In this paper, a review of the current state of knowledge and an outline of some of the outstanding questions that still need to be addressed is provided, based on discussions at a workshop hosted by the Albert Einstein Institute in Golm, Germany.
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Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes
Krzysztof Belczynski,J. Klencki,C. E. Fields,A. Olejak,A. Olejak,Emanuele Berti,Georges Meynet,Chris L. Fryer,Daniel E. Holz,Richard O'Shaughnessy,Duncan A. Brown,Tomasz Bulik,Shing-Chi Leung,Shing-Chi Leung,Ken'ichi Nomoto,Piero Madau,Raphael Hirschi,Raphael Hirschi,Etienne A. Kaiser,Samuel Jones,S. Mondal,Martyna Chruslinska,P. Drozda,Davide Gerosa,Zoheyr Doctor,Zoheyr Doctor,Mirek Giersz,Sylvia Ekström,Cyril Georgy,Abbas Askar,Vishal Baibhav,Daniel Wysocki,T. Natan,Will M. Farr,Grzegorz Wiktorowicz,M. Coleman Miller,Ben Farr,Jean-Pierre Lasota,Jean-Pierre Lasota +38 more
TL;DR: In this article, the authors proposed three models of angular momentum transport in massive stars: a mildly efficient transport by meridional currents, an efficient transport implemented in the MESA code, and a very efficient transport to calculate natal BH spins.