Results 151 to 160 of about 4,916 (215)
Magnetohydrodynamic Simulations of Accretion onto a Star in the “Propeller” Regime [PDF]
, 2003 M. M. Romanova +3 more
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The Evolution of Substructure during Star Cluster Assembly
The Astrophysical JournalStar cluster formation and assembly occur inside filamentary and turbulent molecular clouds, which imprint both spatial and kinematic substructure on the young cluster.
Edwin Laverde-Villarreal +3 more
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Magnetohydrodynamic Numerical Simulations of Solar X-Ray Jets Based on the Magnetic Reconnection Model That Includes Chromospheric Evaporation [PDF]
, 2003 Takehiro Miyagoshi, T. Yokoyama
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Magnetically Arrested Circumbinary Accretion Flows
The Astrophysical Journal LettersBinary systems with comparable masses and a surrounding accretion disk can accrete gas through spiral accretion streams penetrating the central cavity formed by tidal interactions.
Elias R. Most, Hai-Yang Wang
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Magnetohydrodynamic Simulations of the Formation of Cold Fronts in Clusters of Galaxies Including Heat Conduction [PDF]
, 2004 N. Asai, Naoya Fukuda, Ryōji Matsumoto
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Dynamical Inference from Polarized Light Curves of Sagittarius A*
The Astrophysical JournalPolarimetric light curves of Sagittarius A* (Sgr A*) sometimes exhibit loops in the Stokes Q and U plane over time, often interpreted as orbiting hotspot motion. In this work, we apply the differential geometry of planar curves to develop a new technique
Angelo Ricarte +5 more
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Probing Physics of Magnetohydrodynamic Turbulence Using Direct Numerical Simulation
, 1998 Mahendra K. Verma, Gaurav Dar
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A Comparison of the Minimum Current Corona to a Magnetohydrodynamic Simulation of Quasi‐Static Coronal Evolution [PDF]
, 2004 D. W. Longcope, Tetsuya Magara
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