Survey in the Taurus Dark Clouds Alisher S. Hojaev, PASA, 15 (1), 152
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Next Section: Introduction
Some Results of an H
Survey in the Taurus Dark Clouds
Alisher S. Hojaev 
Ulugbek Astronomical Institute, Uzbek Academy of Sciences Astronomicheskaya street, 33, Tashkent 700052, Uzbekistan, Email: hojaev@saturn.silk.org
Abstract:
From a series of 4.degree objective-prism plates obtained on the 1m Schmidt telescope of the Byurakan astrophysical observatory 20 new H emission line stars were found. The intensity of H emission line was evaluated for these stars. An additional sample of probable H emission stars was also found. We present here details and some observational features of these stars. The total number of H emission line stars estimated for the surveyed area is about 80.
Keywords: objective prism survey; H objects; Pre-Main-Sequence stars
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