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Non-ideal magnetohydrodynamics versus turbulence II: Which is the dominant process in stellar core formation?
Monthly Notices of the Royal Astronomical Society ( IF 4.7 ) Pub Date : 2020-05-28 , DOI: 10.1093/mnras/staa1340
James Wurster 1, 2 , Benjamin T Lewis 3
Affiliation  

Funding: JW acknowledges support from the European Research Council under the European Community’s Seventh Framework Programme (FP7/2007- 2013 grant agreement no. 339248), and from the University of St Andrews. BTL acknowledges the support of the National Aeronautics and Space Administration (NASA) through grant NN17AK90G and from the National Science Foundation (NSF) through grants no. 1517488 and PHY-1748958.

中文翻译:

非理想磁流体动力学与湍流 II:哪个是恒星核心形成的主要过程?

资金:JW 感谢欧洲研究理事会根据欧洲共同体第七框架计划(FP7/2007-2013 赠款协议编号 339248)和圣安德鲁斯大学的支持。BTL 通过拨款 NN17AK90G 和美国国家科学基金会 (NSF) 通过拨款 17AK90G 对美国国家航空航天局 (NASA) 的支持表示感谢。1517488 和 PHY-1748958。
更新日期:2020-05-28
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