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

Author： Tambovtseva L. V.   Grinin V. P.   Weigelt G.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|562|issue|A104-A104

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.562, Iss.issue, 2014-02, pp. : A104-A104

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