An analysis of the orbital periods of some eclipsing binaries suspected to be in the pre-main sequence contraction phase of evolution-Reference-Cited by-同舟云学术

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An analysis of the orbital periods of some eclipsing binaries suspected to be in the pre-main sequence contraction phase of evolution

Published:1981-03 Issue:1 Volume:2 Page:29-41
ISSN:0250-6335
Container-title:Journal of Astrophysics and Astronomy
language:en
Short-container-title:J Astrophys Astron

Author:

Panchatsaram T.,Abhyankar K. D.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF02714240.pdf

Reference46 articles.

1. Baglow, R. L. 1952,Pub. David Dunlap Obs.,2, ’No. 1.

2. Bakos, G. A., Tremko, J. 1973,Bull. astr. Inst. Csl.,24, 304.

3. Blanco, C., Criztaldi, S. 1974,Publ. astr. Soc. Pacific,86, 187.

4. Cester, B., Fedel, B., Giuricin, G., Mardirossian, F., Mezzetti, M., Predolin, F. 1979,Mem. Soc. astr. Ital.,50, 551.

5. Chaubey, U. S. 1979,Astrophys. Sp. Sci.,63, 247.

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Spin-up and hot spots can drive mass out of a binary;Astronomy & Astrophysics;2008-07-09

2. A Study of the Orbital Periods of 22 Eclipsing Binaries;International Astronomical Union Colloquium;1982

3. A Study of the Orbital Periods of 22 Eclipsing Binaries;Binary and Multiple Stars as Tracers of Stellar Evolution;1982

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