Accretion variability in young, low-mass stellar systems
Through the study of accretion onto the young, low-mass stars known as T Tauri Stars (TTS), we can better understand the formation of our solar system. Gas is funneled along stellar magnetic field lines into magnetospheric accretion columns where it reaches free-fall velocities and shocks at the ste...
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| Language: | en_US |
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2021
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| Online Access: | https://hdl.handle.net/2144/42027 |