Abstract
The distribution of B stars in the vicinity of nine southern, long-period (P > 11 days) Cepheids is studied on the basis of U, B, V data. The parameters Q, the normal color indices (B — V)0 and (U — B)0, the color excesses E(B — V), the spectral types, and the distance moduli of these stars are determined.
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Translated from Astrofizika, Vol. 40. No. 4, pp. 573–580, October-December, 1997.
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Hovhannessian, R.K. Distribution of B stars in the directions of some southern cepheids. Astrophysics 40, 373–378 (1997). https://doi.org/10.1007/BF03036026
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DOI: https://doi.org/10.1007/BF03036026