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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Journal ArticleDOI
Golden galactic binaries for LISA: mass-transferring white dwarf black hole binaries
TL;DR: In this article, the evolution and gravitational wave emission of white dwarf -black hole accreting binaries with a semi-analytical model is studied. But the model is restricted to binary systems.
Proceedings ArticleDOI
The future of high angular resolution x-ray astronomy
Paul Gorenstein,Webster Cash,Neil Gehrels,Keith C. Gendreau,John Krizmanic,M. Coleman Miller,Christopher S. Reynolds,Rita M. Sambruna,Gerald K. Skinner,Gerald K. Skinner,Robert E. Streitmatter,David L. Windt +11 more
TL;DR: In this article, a Fresnel zone plate is paired with a refractive lens such that their intrinsic chromatic aberrations cancel to 1st order at a specific energy. But the resolution of Chandra is close to the practical limit of grazing incidence telescopes.
Journal ArticleDOI
NICER Detection of Thermal X-Ray Pulsations from the Massive Millisecond Pulsars PSR J0740+6620 and PSR J1614-2230
Michael T. Wolff,Sebastien Guillot,Sebastien Guillot,Slavko Bogdanov,Paul S. Ray,Matthew Kerr,Zaven Arzoumanian,Keith C. Gendreau,M. Coleman Miller,Alexander J. Dittmann,Wynn C. G. Ho,Lucas Guillemot,Lucas Guillemot,Ismaël Cognard,Ismaël Cognard,Gilles Theureau,Gilles Theureau,Gilles Theureau,Kent S. Wood +18 more
TL;DR: The detection of X-ray pulsations from the rotation-powered millisecond-period pulsars PSR J0740+6620 and PSRJ1614−2230, two of the most massive neutron stars known, using observations with the Neutron Star Interior Composition Explorer (NICER) was reported in this article.
Journal ArticleDOI
Reionization Constraints on the Contribution of Primordial Compact Objects to Dark Matter
TL;DR: In this paper, it was shown that accretion onto these objects produces substantial ionization in the early universe, with an optical depth to Thomson scattering out to z=1100 of approximately tau=2-4 [f_CO\epsilon{-1}(M/Msun)]^{1/2} (H_0/65)^{-1}, where f_CO is the accretion efficiency
Journal ArticleDOI
A strong test of the dark matter origin of a TeV electron excess using icecube neutrinos
TL;DR: In this paper, a non-astrophysical scenario in which dark matter particles annihilate or decay in a local clump has been invoked to explain the tentative excess in the electron spectrum at 1.4 TeV reported by the DArk Matter Particle Explorer (DAMPE).