Julian H. Krolik
14 ta ish
Johns Hopkins University
DISK FORMATION VERSUS DISK ACCRETION—WHAT POWERS TIDAL DISRUPTION EVENTS?
Tsvi Piran, Gilad Svirski, Julian H. Krolik +2
MaqolaOchiq kirish20155 iqtibosABIX-RAY POLARIZATION FROM ACCRETING BLACK HOLES: THE THERMAL STATE
Jeremy D. Schnittman, Julian H. Krolik
MaqolaOchiq kirish20095 iqtibosABIDEPENDENCE OF INNER ACCRETION DISK STRESS ON PARAMETERS: THE SCHWARZSCHILD CASE
Scott C. Noble, Julian H. Krolik, John F. Hawley
MaqolaOchiq kirish20103 iqtibosABIFe Kα PROFILES FROM SIMULATIONS OF ACCRETING BLACK HOLES
Brooks E. Kinch, Jeremy D. Schnittman, T. R. Kallman +1
MaqolaOchiq kirish20163 iqtibosABIQuasiperiodic Erupters: A Stellar Mass-transfer Model for the Radiation
MaqolaOchiq kirish20222 iqtibosABIElectromagnetic Emission from Supermassive Binary Black Holes Approaching Merger
Stéphane d’Ascoli, Scott C. Noble, Dennis Bowen +3
MaqolaOchiq kirish20182 iqtibosABIDIRECT CALCULATION OF THE RADIATIVE EFFICIENCY OF AN ACCRETION DISK AROUND A BLACK HOLE
Scott C. Noble, Julian H. Krolik, John F. Hawley
MaqolaOchiq kirish20092 iqtibosABI