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The light variability of BD+25°2511

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Abstract

Photometry of the spectroscopic binary BD+25°2511 obtained during the 1981, 1982, and 1983 observing seasons shows that it is a variable with a period of about 3.5 days.

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References

  • Eggen, O. J.: 1978,Inf. Bull. Var. Stars, No. 1426.

  • Raveendran, A. V., Mekkaden, M. V., and Mohin, S.: 1982,Monthly Notices Roy. Astron. Soc. 199, 707.

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Authors and Affiliations

  1. Indian Institute of Astrophysics Bangalore, India

    A. V. Raveendran

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  1. A. V. Raveendran
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Raveendran, A.V. The light variability of BD+25°2511. Astrophys Space Sci 99, 171–173 (1984). https://doi.org/10.1007/BF00650242

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  • DOI: https://doi.org/10.1007/BF00650242

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