Modeling the Break in the Specific Angular Momentum within the Envelope–Disk Transition Zone
The observations of protostellar systems show a transition in the radial profile of specific angular momentum (and rotational velocity), as evolving from $j\sim {\rm{constant}}$ ( v _ϕ ∼ r ^−1 ) in the infalling-rotating envelope to j ∝ r ^1/2 ( v _ϕ ∼ r ^ −1/2 ) in the Keplerian disk. We empl...
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| Auteurs principaux: | , , , , |
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| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
IOP Publishing
2026-01-01
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| Collection: | The Astrophysical Journal |
| Sujets: | |
| Accès en ligne: | https://doi.org/10.3847/1538-4357/ae4725 |
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