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Cited article:

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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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THE MASS DEPENDENCE BETWEEN PROTOPLANETARY DISKS AND THEIR STELLAR HOSTS

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S. Hubrig, M. Schöller, I. Ilyin, B. Wolff, C.R. Cowley, M.A. Pogodin, R.V. Yudin, B. Stelzer and Z. Mikulášek
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Characterising the magnetic fields of the Herbig Ae/Be stars HD 97048, HD 150193, HD 176386, and MWC 480

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TOWARD UNDERSTANDING THE B[e] PHENOMENON. III. PROPERTIES OF THE OPTICAL COUNTERPART OF IRAS 00470+6429

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SPECTROPOLARIMETRIC OBSERVATIONS OF HERBIG AE/BE STARS. II. COMPARISON OF SPECTROPOLARIMETRIC SURVEYS: HAEBE, BE AND OTHER EMISSION-LINE STARS

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Structure of the inner regions of the circumstellar gas envelopes around young hot stars. II. The new cycle of spectral activity of the Herbig Ae star HD 31648

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Spectropolarimetry of the Hα Line in Herbig Ae/Be Stars

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A search for strong, ordered magnetic fields in Herbig Ae/Be stars

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Large-scale variability in the profiles of Hα and Hβ in the spectrum of the Herbig B8e star MWC 419 and a model interpretation of it

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Influence of stellar wind on the long-term variability of the Hα emission line. The case of the Herbig Ae-star HD 31648

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