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Two dimensional spectral classification of stars in the neighborhood of the stellar cluster NGC 2175

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Abstract

Spectral classifications of 1224 O-M stars in different luminosity classes in the neighborhood of NGC 2175 are presented. The classifications are based on low dispersion objective prism spectra. B-V and U-B data for 106 of the 1224 stars are used to obtain MK classifications using the photometric Q method.

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Authors and Affiliations

  1. V. A. Ambartsumyan Byurakan Astrophysical Observatory, Byurakan, Armenia

    R. Kh. Hovhannesian & R. A. Epremian

  2. E. K. Kharadze Abastumani National Astrophysical Observatory, Abastumani, Georgia

    M. D. Metreveli

Authors
  1. R. Kh. Hovhannesian
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  2. R. A. Epremian
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  3. M. D. Metreveli
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Corresponding author

Correspondence to R. Kh. Hovhannesian.

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Translated from Astrofizika, Vol. 51, No. 2, pp. 339–341 (May 2008).

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Hovhannesian, R.K., Epremian, R.A. & Metreveli, M.D. Two dimensional spectral classification of stars in the neighborhood of the stellar cluster NGC 2175. Astrophysics 51, 276–278 (2008). https://doi.org/10.1007/s10511-008-9001-0

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  • DOI: https://doi.org/10.1007/s10511-008-9001-0

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