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Cited article:

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Modeling of Hydrogen Emission Lines in the Spectrum of UX Ori in Its Bright State and during Eclipses

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Dynamics of wind and the dusty environments in the accreting T Tauri stars RY Tauri and SU Aurigae

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Hydrogen lines as a diagnostic tool for studying multicomponent emitting regions in hot young stars: magnetosphere, X-wind, and disk wind

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AA Tauri’s sudden and long-lasting deepening: enhanced extinction by its circumstellar disk

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Geometry and velocity structure of HD 44179’s bipolar jet

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