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Birth of a relativistic outflow in the unusual γ-ray transient Swift J164449.3+573451.A 15.65-solar-mass black hole in an eclipsing binary in the nearby spiral galaxy M 33.Generation of primordial magnetic fields on linear overdensity scales.Cosmological Applications of Gravitational LensingHarmony in Electrons: Cyclotron and Synchrotron Emission by Thermal Electrons in a Magnetic FieldThe mass of the black hole in Cygnus X-1Spectra and Light Curves of Gamma-Ray Burst AfterglowsBlack holes in astrophysicsAdvection-dominated accretion: A self-similar solutionThe spin of the black hole microquasar XTE J1550−564 via the continuum-fitting and Fe-line methodsThe Spin of the Near‐Extreme Kerr Black Hole GRS 1915+105The event horizon of Sagittarius A*Advection-dominated accretion and the black hole event horizonThe Rates of Type I X‐Ray Bursts from Transients Observed withRXTE: Evidence for Black Hole Event HorizonsOn the mass distribution and birth masses of neutron starsThe extreme spin of the black hole in Cygnus X-1Evidence for the black hole event horizonMaximum Likelihood Cluster ReconstructionThe cool accretion disk in ESO 243-49 HLX-1: further evidence of an intermediate-mass black holeX-ray polarimetry with the Polarization Spectroscopic Telescope Array (PolSTAR)A Hydrogen Atmosphere Spectral Model Applied to the Neutron Star X7 in the Globular Cluster 47 TucanaeLocating the intense interstellar scattering towards the inner GalaxyThe event horizon of M87Origin of the Soft Excess in X‐Ray PulsarsThe Lens Parallax Method: Determining Redshifts of Faint Blue Galaxies through Gravitational LensingKinetic inhibition of magnetohydrodynamics shocks in the vicinity of a parallel magnetic fieldA parallax distance to the microquasar GRS 1915+105 and a revised estimate of its black hole massConfirmation via the continuum-fitting method that the spin of the black hole in Cygnus X-1 is extremeHow Much Mass Do Supermassive Black Holes Eat in Their Old Age?Spectra and Line Profiles of FU Orionis Objects: Comparisons between Boundary Layer Models and ObservationsBoundary Layers in Pre-Main-Sequence Accretion DisksGlobular clusters and dark satellite galaxies through the stream velocityFast variability and millimeter/IR flares in GRMHD models of Sgr A* from strong-field gravitational lensingHost galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNsThe luminosity of particle beams from thick accretion discsTwo-phase spectral modelling of 1E1740.7-2942Extreme brightness temperatures and refractive substructure in 3C273 with RadioAstronOptical and X-ray luminosities of expanding nebulae around ultraluminous X-ray sourcesWhat Is the Accretion Rate in NGC 4258?Advection‐dominated Accretion Model of Sagittarius A*: Evidence for a Black Hole at the Galactic Center
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description
Theoretical astrophysicist at Harvard University
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astrofysicus
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name
Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Narayan R
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Narayan R.
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R Narayan
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R. Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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Ramesh Narayan
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