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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The Shapes of Atomic Lines from the Surfaces of Weakly Magnetic Rotating Neutron Stars and Their Implications
TL;DR: In this paper, the authors investigated the information about neutron star structure and the geometry of the emission region that can be obtained by analyzing the profiles of atomic lines formed at the surface of the star.
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Disk-accreting magnetic neutron stars as high-energy particle accelerators
TL;DR: In this article, the authors argue that large conduction currents will cause microscopic and macroscopic instabilities in the magnetosphere, which will accelerate charged particles to very high energies.
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Astrophysics: Weighing in on neutron stars
TL;DR: The observed range of neutron star masses has hitherto been too narrow to rule out many predictions of 'exotic' non-nucleonic components, but this pulsar weighs in at around two solar masses, ruling out almost all currently proposed equations of state involving exotic hyperon or boson condensates.
Journal Article
Decadal Survey White Paper: Probing Stellar Dynamics in Galactic Nuclei
M. Coleman Miller,Tal Alexander,Pau Amaro-Seoane,Aaron J. Barth,Curt Cutler,Jonathan R. Gair,Clovis Hopman,David Merritt,E. Sterl Phinney,Douglas O. Richstone +9 more
TL;DR: In this paper, the authors show that future low-frequency gravitational wave observations, alone or in combination with electromagnetic data, will open up unique windows to the processes of supermassive black holes (SMBHs).
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A Sensitive Search for Supernova Emission Associated with the Extremely Energetic and Nearby GRB 221009A
Gokul P. Srinivasaragavan,B. O'Connor,S. Bradley Cenko,Alexander J. Dittmann,Sheng Yang,Jesper Sollerman,G. C. Anupama,Sudhanshu Barway,Varun Bhalerao,Harsha S. Kumar,V. M. Swain,Erica Hammerstein,Isiah Holt,Shreya Anand,Igor Andreoni,Michael W. Coughlin,Simone Dichiara,Avishay Gal-Yam,M. Coleman Miller,Jaime Soon,Roberto Soria,J. M. Durbak,J. Gillanders,Sibasish Laha,Anna Moore,F. Ragosta,Eleonora Troja +26 more
TL;DR: In this paper , a phenomenological power-law model for the afterglow and host galaxy estimates from high-resolution Hubble Space Telescope imaging was used to determine the likelihood of an associated supernova contributing excess flux to the optical light curve.