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Investigation of late-type stars in the FBS survey. I. M stars

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Abstract

The spectral subtypes and luminosity classes are given for 15 comparatively faint M stars found on plates of the First Byurakan Spectroscopic Survey. Two of them are classified as M dwarfs. Most of the new M stars are probably Mirids.

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Authors and Affiliations

  1. Byurakan Astrophysical Observatory, Armenia

    H. V. Abrahamian, V. V. Hambarian & K. S. Gigoyan

Authors
  1. H. V. Abrahamian
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  2. V. V. Hambarian
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  3. K. S. Gigoyan
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Additional information

Translated from Astrofizika, Vol. 37, No. 1, pp. 73–82, January–February, 1994.

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Abrahamian, H.V., Hambarian, V.V. & Gigoyan, K.S. Investigation of late-type stars in the FBS survey. I. M stars. Astrophysics 37, 44–50 (1994). https://doi.org/10.1007/BF02113994

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  • DOI: https://doi.org/10.1007/BF02113994

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