Article

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;

Publications of the Astronomical Society of Australiajournal1998en

ABI

Abstract

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.

Topics

Astronomical Observations and Instrumentation Stellar, planetary, and galactic studies Astrophysics and Star Formation Studies

Identifiers

DOI: 10.1071/as98152

Citations and references

Cited by 03 references

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