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Evidence for disks at an early stage in class 0 protostars?
AIMS: The formation epoch of protostellar disks is debated because of the competing roles of rotation, turbulence, and magnetic fields in the early stages of low-mass star formation. Magnetohydrodynamics simulations of collapsing cores predict that rotationally supported disks may form in strongly m...
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| 出版年: | Astron Astrophys |
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| 主要な著者: | , , , , , , , , , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
2017
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| 主題: | |
| オンライン･アクセス: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5683350/ https://ncbi.nlm.nih.gov/pubmed/29142329 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201630187 |
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