On the constancy of the light curve of CC comae-Reference-Cited by-同舟云学术

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On the constancy of the light curve of CC comae

Published:1982-08 Issue:1 Volume:86 Page:107-115
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Breinhorst R. A.,Hoffmann M.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00651833.pdf

Reference5 articles.

1. Hoffmeister, C.: 1964,Astron. Nachr. 288, 49.

2. Kwee, K. K. and van Woerden, H.: 1956,Bull. Astron. Inst. Neth. 12, 327.

3. Rucinski, S. M.: 1976,Publ. Astron. Soc. Pacific 88, 777.

4. Wenzel, W.: 1967,Mitt. Ver�nderliche Sterne Sonneberg 4, 60.

5. Zhukov, G. V.: 1976,Astron. Tsirk., No. 918, 7.

Cited by 8 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. The short-period low-mass binary system CC Com revisited;Astronomische Nachrichten;2011-07

2. Physical parameters of components in close binary systems - VII;Monthly Notices of the Royal Astronomical Society;2010-08-18

3. ORBITAL PERIOD CHANGES AND THEIR EVOLUTIONARY STATUS FOR WEAK-CONTACT BINARIES. II. CC COMAE BERENICES AND BV DRACONIS;The Astronomical Journal;2008-12-10

4. Period Changes of Two W UMa–Type Contact Binaries: RW Comae Berenices and CC Comae Berenices;Publications of the Astronomical Society of the Pacific;2003-06

5. CC Comae - an apparent secular filling factor change;The Astrophysical Journal;1989-08

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