Lyα Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems
T Tauri stars produce broad Ly α emission lines that contribute ∼88% of the total UV flux incident on the inner circumstellar disks. Ly α photons are generated at the accretion shocks and in the protostellar chromospheres and must travel through accretion flows, winds, and jets, the protoplanetary d...
| Published in: | The Astrophysical Journal |
|---|---|
| Main Authors: | , , , , , , , , , , , , , , , , , , , , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2023-01-01
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| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/acaf70 |
