Fluorescent iron lines as a probe of astrophysical black hole systems

CS Reynolds, MA Nowak - Physics Reports, 2003 - Elsevier
With most physicists and astrophysicists in agreement that black holes do indeed exist, the
focus of astrophysical black hole research has shifted to the detailed properties of these …

Particle motion, shadows and thermodynamics of regular black hole in pure gravity

A Ditta, A Bouzenada, G Mustafa, YM Alanazi… - Physics of the Dark …, 2024 - Elsevier
This paper investigates the thermodynamic behaviors and optical properties of regular black
holes within pure gravity theories, notable for their absence of singularities. Using both …

Discerning the physical origins of cosmological gamma-ray bursts based on multiple observational criteria: the cases of z= 6.7 GRB 080913, z= 8.2 GRB 090423, and …

B Zhang, BB Zhang, FJ Virgili, EW Liang… - The Astrophysical …, 2009 - iopscience.iop.org
The two high-redshift gamma-ray bursts, GRB 080913 at z= 6.7 and GRB 090423 at z= 8.2,
recently detected by Swift appear as intrinsically short, hard GRBs. They could have been …

Black hole spin evolution

CF Gammie, SL Shapiro… - The Astrophysical …, 2004 - iopscience.iop.org
We consider a subset of the physical processes that determine the spin j≡ a/M of
astrophysical black holes. These include (1) Initial conditions. Recent models suggest that …

XMM-EPIC observation of MCG-6-30-15: direct evidence for the extraction of energy from a spinning black hole?

J Wilms, CS Reynolds, MC Begelman… - Monthly Notices of …, 2001 - academic.oup.com
Abstract We present XMM-Newton European Photon Imaging Camera (EPIC) observations
of the bright Seyfert 1 galaxy MCG–6-30-15, focusing on the broad Fe K α line at∼ 6 keV …

Ergomagnetosphere, ejection disc, magnetopause in M87–I. Global flow of mass, angular momentum, energy, and current

R Blandford, N Globus - Monthly Notices of the Royal …, 2022 - academic.oup.com
We interpret the 1.3 mm VLBI observations made by the Event Horizon Telescope of the
black hole in M87. It is proposed that, instead of being a torus of accreting gas, the observed …

Multitemperature blackbody spectrum of a thin accretion disk around a Kerr black hole: model computations and comparison with observations

LX Li, ER Zimmerman, R Narayan… - The Astrophysical …, 2005 - iopscience.iop.org
We use a ray-tracing technique to compute the observed spectrum of a thin accretion disk
around a Kerr black hole. We include all relativistic effects such as frame-dragging, Doppler …

Evolution characteristics of the central black hole of a magnetized accretion disc

DX Wang, K Xiao, WH Lei - Monthly Notices of the Royal …, 2002 - academic.oup.com
Evolution characteristics of a Kerr black hole (BH) are investigated by considering the
coexistence of disc accretion with the Blandford–Znajek process (the BZ process) and …

Force-free magnetosphere of an accretion disk-black hole system. II. Kerr geometry

DA Uzdensky - The Astrophysical Journal, 2005 - iopscience.iop.org
We consider a stationary axisymmetric force-free degenerate magnetosphere of a rotating
Kerr black hole surrounded by a thin, Keplerian, infinitely conducting accretion disk. We …

Magnetically torqued neutrino-dominated accretion flows for gamma-ray bursts

WH Lei, DX Wang, L Zhang, ZM Gan… - The Astrophysical …, 2009 - iopscience.iop.org
Recent observations and theoretical work on gamma-ray bursts favor the central engine
model of a Kerr black hole (BH) surrounded by a magnetized neutrino-dominated accretion …