Accretion variability from minute to decade timescales in the classical T Tauri star CR Cha
Context. Classical T Tauri stars are pre-main-sequence stars that are surrounded by a circumstellar disk from which they accrete material. The mass accretion process is essential in the formation of Sun-like stars. Although often described with simple and static models, the accretion process is inhe...
| Main Authors: | , , , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2022
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| Subjects: | |
| Online Access: | View Fulltext in Publisher |