An apparent descriptive method for judging the synchronization of rotation of binary stars-Reference-Cited by-同舟云学术

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An apparent descriptive method for judging the synchronization of rotation of binary stars

Published:2004-09 Issue:3-4 Volume:25 Page:203-211
ISSN:0250-6335
Container-title:Journal of Astrophysics and Astronomy
language:en
Short-container-title:J Astrophys Astron

Author:

Lin-sen Li

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF02702372.pdf

Reference16 articles.

1. Batten, A. H.et al. 1989,Publ. Dom. Astrophys,17, 1–127.

2. Brancewicz, H. K., Dworak, T. Z. 1980,Acta Astronomic a,30(4), 501.

3. Giuricin, G.et al. 1984,A & A,131, 152;135, 393.

4. Kopal, Z. 1959,Close binary system (London: Chapman and Hall) p. 470.

5. Levato, H. 1976,Ap J,203, 680.

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1. Observational investigation of the dynamical tides in massive eccentric binaries;Monthly Notices of the Royal Astronomical Society;2023-10-14

2. Orbit and spin evolution of synchronous binary stars on the main sequence (a theoretical improvement to the analytical method);Research in Astronomy and Astrophysics;2015-10

3. Orbit and spin evolution of synchronous binary stars on the main sequence;Research in Astronomy and Astrophysics;2012-11-22

4. CHEMICAL COMPOSITION OF THE COMPONENTS OF ECLIPSING BINARY STAR ZZ BOOTIS;The Astronomical Journal;2012-06-26

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