Edward Brown
educated at: Ohio State University, University of California, Berkeley
occupation: researcher
official website: www.pa.msu.edu/~ebrown
Articles 87
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Consistent accretion-induced heating of the neutron-star crust in MXB 1659−29 during two different outbursts
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Dense matter with eXTP
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Rapid Neutrino Cooling in the Neutron Star MXB 1659-29
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Multi-messenger Observations of a Binary Neutron Star Merger
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The LOFT mission concept: a status update
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The thermal state of KS 1731-260 after 14.5 years in quiescence
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Dead or Alive? Long-term evolution of SN 2015bh (SNhunt275)
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Urca cooling pairs in the neutron star ocean and their effect on superbursts
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Constraining the properties of neutron star crusts with the transient low-mass X-ray binary Aql X-1
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A tracer method for computing Type Ia supernova yields: burning model calibration, reconstruction of thickened flames, and verification for planar detonations
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On measuring the metallicity of a type Ia supernova's progenitor
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Massive stars exploding in a He-rich circumstellar medium – IV. Transitional Type Ibn supernovae
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A strong shallow heat source in the accreting neutron star MAXI J0556-332
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Early ultraviolet emission in the Type Ia supernova LSQ12gdj: No evidence for ongoing shock interaction
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The Large Observatory for x-ray timing
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Carbon synthesis in steady-state hydrogen and helium burning on accreting neutron stars
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Probing the crust of the neutron star in EXO 0748-676
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A way forward in the study of the symmetry energy: experiment, theory, and observation
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On silicon group elements ejected by supernovae type Ia
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Strong neutrino cooling by cycles of electron capture and β- decay in neutron star crusts.
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Continued neutron star crust cooling of the 11 hz X-ray pulsar in Terzan 5: a challenge to heating and cooling models?
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Modules for experiments in stellar astrophysics (MESA): planets, oscillations, rotation, and massive stars
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A change in the quiescent X-ray spectrum of the neutron star low-mass X-ray binary MXB 1659-29
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The neutron star mass-radius relation and the equation of state of dense matter
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Low-temperature triple-alpha rate in a full three-body nuclear model.
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LOFT: the Large Observatory For X-ray Timing
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On Simulating Type Ia Supernovae
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Evaluating systematic dependencies of type Ia supernovae: the influence of central density
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Does the12C+12C fusion reaction trigger superburst?
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Correlation between the12C+12C,12C+13C, and13C+13C fusion cross sections
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ERRATUM: “THE VARIABLE QUIESCENT X-RAY EMISSION OF THE NEUTRON STAR TRANSIENT XTE J1701–462” (2011, ApJ, 736, 162)
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The variable quiescent X-ray emission of the transient neutron star XTE J1701-462
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