Protostellar Disk Formation Regimes: Angular Momentum Conservation versus Magnetic Braking
Protostellar disks around young protostars exhibit diverse properties, with their radii ranging from less than ten to several hundred astronomical units. To investigate the mechanisms shaping this disk radius distribution, we compiled a sample of 27 Class 0 and I single protostars with resolved disk...
| मुख्य लेखकों: | , |
|---|---|
| स्वरूप: | लेख |
| भाषा: | English |
| प्रकाशित: |
IOP Publishing
2024-01-01
|
| श्रृंखला: | The Astrophysical Journal Letters |
| विषय: | |
| ऑनलाइन पहुंच: | https://doi.org/10.3847/2041-8213/ad7263 |