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20162026
most citedFe K Profiles from Simulations of Accreting Black Holes

28 citations · 73 across the 8 of their papers we have counts for

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astro-ph.HE2026

Thermal and non-thermal emission from supermassive black hole circumbinary disks: Disks, Coronae, Streams, and Cavities

Chris Nagele, Julian H. Krolik, Brooks E. Kinch +4

The search for electromagnetic signals from supermassive black hole (SMBH) binary systems is one of the cornerstones of multi-messenger astrophysics, complementing gravitational wa…

astro-ph.HE2026

Simulation-Based Prediction of Black Hole Fe K Line Profiles

Chris Nagele, Julian H. Krolik, Brooks E. Kinch +1

One of the most useful spectral diagnostics of accreting black hole systems is the Fe K fluorescence line. Detected in many systems, it is often used to estimate the black hole…

astro-ph.HE2026

Simulation-Based Prediction of Black Hole Spectra: From to

Chris Nagele, Julian H. Krolik, Rongrong Liu +2

It has long been thought that black hole accretion flows are driven by magnetohydrodynamic (MHD) turbulence, and there are now many general relativistic global simulations illustra…

astro-ph.HE2024

Simulation-Based Prediction of Black Hole X-ray Spectra and Spectral Variability

Rongrong Liu, Chris Nagele, Julian H Krolik +2

Data derived from general relativistic magnetohydrodynamic simulations of accretion onto black holes can be used as input to a postprocessing scheme that predicts the radiated spec…

astro-ph.HE2021★ 27 cited

Spin and Accretion Rate Dependence of Black Hole X-Ray Spectra

Brooks E. Kinch, Jeremy D. Schnittman, Scott C. Noble +2

We present a survey of how the spectral features of black hole X-ray binary systems depend on spin, accretion rate, viewing angle, and Fe abundance when predicted on the basis of f…

astro-ph.HE2020★ 16 cited

Inverse Compton Cooling in the Coronae of Simulated Black Hole Accretion Flows

Brooks E. Kinch, Scott C. Noble, Jeremy D. Schnittman +1

We present a formulation for a local cooling function to be employed in the diffuse, hot corona region of 3D GRMHD simulations of accreting black holes. This new cooling function c…

astro-ph.HE2018★ 2 cited

Predicting Stellar-Mass Black Hole X-ray Spectra from Simulations

Brooks E. Kinch, Jeremy D. Schnittman, Timothy R. Kallman +1

We describe results from a new technique for the prediction of complete, self-consistent X-ray spectra from three-dimensional General Relativistic magnetohydrodynamic (GRMHD) simul…

astro-ph.HE2016★ 28 cited

Fe K Profiles from Simulations of Accreting Black Holes

Brooks E. Kinch, Jeremy D. Schnittman, Timothy R. Kallman +1

We present first results from a new technique for the prediction of Fe K profiles directly from general relativistic magnetohydrodynamic (GRMHD) simulations. Data from a GRMHD s…