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• W3100350042 abstract "Context. Models of magnetically-driven accretion and outflows reproduce many observational properties of T Tauri stars. This concept is not well established for the more massive Herbig Ae/Be stars." @default.
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• W3100350042 date "2016-07-22" @default.
• W3100350042 modified "2023-10-03" @default.
• W3100350042 title "Spectroscopic signatures of magnetospheric accretion in Herbig Ae/Be stars" @default.
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• W3100350042 doi "https://doi.org/10.1051/0004-6361/201628361" @default.
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