Some Results of an H<i>α</i> Survey in the Taurus Dark Clouds
A. S. HojaevUlugbek Astronomical Institute, Uzbek Academy of Sciences, Astronomicheskaya St 33, Tashkent 700052, Uzbekistan;
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Аннотация
Abstract From a series of 4° objective-prism plates obtained on the 1 m Schmidt telescope of the Byurakan Astrophysical Observatory, 20 new H α emission line stars were found. The intensity of H α emission line was evaluated for these stars. An additional sample of probable H α emission stars was also found. We present here details and some observational features of these stars. The total number of H α emission line stars estimated for the surveyed area is about 80.
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