Abstract
The results of investigations of new faint M and C type stars discovered on the plates of the First Byurakan Spectral Sky Survey are reported. Among 161 newly discovered stars, 98 are identified with unknown IRAS point sources. It is probable that the majority of new M stars are Mirids according to their distributions on the IRAS color—color diagram. For J stars, a correlation between EW(C2 + CN) and EW(C2(0,1)) is found.
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Published in Astrofizika, Vol. 38, No. 4, pp. 543–548, October–December, 1995.
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Gigoyan, K.S., Hambarian, V.V. & Abrahamian, H.V. The first Byurakan spectral sky survey. Investigations of stars of late M and C spectral classes. Astrophysics 38, 300–302 (1995). https://doi.org/10.1007/BF02044698
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DOI: https://doi.org/10.1007/BF02044698