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机译:AB Initio Horizo n-Scale模拟Sagittarius A *由Stellar Winds喂养的磁阻
Univ Calif Santa Barbara Kavli Inst Theoret Phys Kohn Hall Santa Barbara CA 93107 USA;
Univ Calif Santa Barbara Kavli Inst Theoret Phys Kohn Hall Santa Barbara CA 93107 USA;
Univ Calif Berkeley Dept Astron 501 Campbell Hall Berkeley CA 94720 USA;
Inst Adv Study 1 Einstein Dr Princeton NJ 08540 USA;
Galactic center; Magnetohydrodynamics; Astrophysical fluid dynamics; Astrophysical black holes; Accretion; General relativity; Wolf-Rayet stars; Stellar winds; Magnetohydrodynamical simulations;
机译:带有Wind Infall的吸积磁盘演进。二。三维流体动力学模拟的结果及其在射手座A *上的说明性应用
机译:带有防风雨的增生盘进化。二。三维流体动力学模拟结果的应用
机译:增粘实心风。二。星形风转矩的数值解
机译:合金热力学从头模拟中的有限温度,磁性和多体效应
机译:吸积盘和恒星风的天体流体动力学的概念发展
机译:从头算分子动力学模拟揭示石墨烯单空位磁态的热力学稳定性
机译:AB Initio Horizo n-Scale模拟射手座A *由Stellar Winds喂养
机译:铁基块体非晶态金属的电子和磁性结构:从头算方法