A photometric study of the contact binary XY Boo

Author:

Awadalla Nabil S.,Yamasaki A.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference10 articles.

1. Binnendijk, L.: 1971,Astron. J. 76, 923.

2. Carbon, D. F. and Gingerich, O.: 1969, in O. Gingerich (ed.),Theory and Observation of Normal Stellar Atmospheres, MIT Press Cambridge, U.S.A.

3. Hinderer, F.: 1960,J. Obs. 43, 161.

4. Hoffmeister, C.: 1935,Astron. Nachr. 255, 401.

5. Kitamura, M. and Yamasaki, A.: 1984,Ann. Tokyo Astron. Obs. 2nd Ser. 20, 35.

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1. Orbital Period Analysis of Four Eclipsing Binaries XY Boo, RW Com, MR Del and AK Her;ACTA ASTRONOM;2020

2. Phenomenological modelling of eclipsing system light curves;Astronomy & Astrophysics;2015-11-13

3. UNIFICATION OF BINARY STAR EPHEMERIS SOLUTIONS;The Astrophysical Journal;2013-12-20

4. On the origin of W UMa type contact binaries – a new method for computation of initial masses;Monthly Notices of the Royal Astronomical Society;2013-02-05

5. Angular momentum and mass evolution of contact binaries;Monthly Notices of the Royal Astronomical Society;2008-10

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