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Some Results of an Hα Survey in the Taurus Dark Clouds

Published online by Cambridge University Press:  16 May 2016

Alisher S. Hojaev
Alisher S. Hojaev*
Affiliation:
Ulugbek Astronomical Institute, Uzbek Academy of Sciences, Astronomicheskaya St 33, Tashkent 700052, Uzbekistan; hojaev@saturn.silk.org
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Abstract

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From a series of 4° objective-prism plates obtained on the 1 m Schmidt telescope of the Byurakan Astrophysical Observatory, 20 new Hα emission line stars were found. The intensity of Hα emission line was evaluated for these stars. An additional sample of probable Hα emission stars was also found. We present here details and some observational features of these stars. The total number of Hα emission line stars estimated for the surveyed area is about 80.

Keywords

objective prism surveyHαobjectspre-main-sequence stars
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 15 , Issue 1 , 1998 , pp. 152 - 154
Copyright
Copyright © Astronomical Society of Australia 1998

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