Results 111 to 120 of about 2,051 (189)
Magnetohydrodynamic Simulations of Accretion onto a Star in the “Propeller” Regime [PDF]
, 2003 M. M. Romanova +3 more
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The Astrophysical JournalTurbulent diffuse molecular clouds can exhibit complicated morphologies caused by the interactions among radiation, chemistry, fluids, and fields.
Nannan Yue +4 more
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Photoelectric Heating and [C
, 2003 M. Juvela, Paolo Padoan, Raúl Jiménez
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Three‐dimensional Magnetohydrodynamic Simulations of Radiatively Inefficient Accretion Flows [PDF]
, 2003 I. V. Igumenshchev +2 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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