An analysis of the light changes of the eclipsing binary XY ceti in the frequency-domain

Author:

Srivastava R. K.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference23 articles.

1. Al-Naimiy, E., Budding, E., Jassur, D., and Sadik, A. R.: 1978,Inf. Bull. Var. Stars, No. 1415.

2. Arp, H. C.: 1958, inHandb. d. Phys. 51, 83.

3. Budding, E.: 1973,Astrophys. Space Sci. 22, 87.

4. Hill, G., Hilditch, R. W., Younger, R., and Fisher, W. A.: 1975,Mem. Roy. Astron. Soc. 79, 131.

5. Hilditch, R. W. and Hill, G.: 1975,Mem. Roy. Astron. Soc. 79, 107.

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1. Absolute dimensions of detached eclipsing binaries - II. The metallic-lined system XY Ceti;Monthly Notices of the Royal Astronomical Society;2011-05-02

2. Calculation of tidal-evolution constants for close binary systems;Kinematics and Physics of Celestial Bodies;2011-04

3. Synchronization and circularization in early-type binaries on main sequence;Monthly Notices of the Royal Astronomical Society;2010-01-01

4. New absolute magnitude calibrations for detached binaries;Astronomische Nachrichten;2008-10

5. Period study of XY Ceti;Astrophysics and Space Science;1988

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