Period Change of CU Pegasi

Details Period Change of CU Pegasi Period Change of CU Pegasi

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.305..385p&link_type=abstract

Astrophysics and Space Science, Volume 305, Issue 4, pp.385-388

Astronomy and Astrophysics

Astrophysics

Binary Stars, Eclipsing Binaries, Period Changes, Individual &Ndash, Cu Peg

Scientific paper

On the basis of the published times of minima and our own observations, we analysed the period change of the Algol-type eclipsing binary CU Pegasi. Over almost seventy years of observations, the parabolic period change has been clearly seen as dP/dt = 1.38 × 10-6 d/year. The estimated mass transfer in the system is about 1 × 10-7 MM&sun;/year.

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