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Modeling of Hydrogen Emission Lines in the Spectrum of UX Ori in Its Bright State and during Eclipses
Authors:Tambovtseva  L V  Grinin  V P  Dmitriev  D V
Institution:1.Central (Pulkovo) Astronomical Observatory, Russian Academy of Sciences, 196140, St. Petersburg, Russia
;2.V.V. Sobolev Astronomical Institute, St. Petersburg State University, Petrodvorets, 196140, St. Petersburg, Russia
;
Abstract:Astronomy Reports - The hydrogen spectrum of the UX Ori-type star is modeled in a bright state and during an eclipse by an opaque dusty fragment of its own protoplanetary disk. The disk wind is...
Keywords:
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