Cloud Dissipation and Disk Wind in the Late Phase of Star Formation
We perform a long-term simulation of star and disk formation using three-dimensional nonideal magnetohydrodynamics. The simulation starts from a prestellar cloud and proceeds through the long-term evolution of the circumstellar disk until ∼1.5 × 10 ^5 yr after protostar formation. The disk has size...
| 發表在: | The Astrophysical Journal |
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| Main Authors: | , |
| 格式: | Article |
| 語言: | 英语 |
| 出版: |
IOP Publishing
2024-01-01
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| 主題: | |
| 在線閱讀: | https://doi.org/10.3847/1538-4357/ad4997 |