BV observations of W UMa-type binaries: CK Boo, BI CVn, and AH Vir

Date

1987-7

Author

Demircan, Osman

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Photoelectric BV observations of W UMa-type binaries CK Boo, BI CVn, and AH Vir are presented, and light curve variations and shifts of minima are discussed in the context of stellar activity and mass transfer. The O−C increments in three systems were found to be 0.08, 0.80, and 0.60 s per revolution, respectively. The new ephemeris for the future observations were also found.

Subject Keywords

Space and Planetary Science, Astronomy and Astrophysics

URI

https://hdl.handle.net/11511/51959

Journal

Astrophysics and Space Science

DOI

https://doi.org/10.1007/bf00644471

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Department of Physics, Article

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Citation Formats

O. Demircan, “BV observations of W UMa-type binaries: CK Boo, BI CVn, and AH Vir,” Astrophysics and Space Science, pp. 169–174, 1987, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/51959.