EB-type contact binary do cas with a large temperature difference

Author:

Oh Kyu-Dong,Ahn Young-Sook

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference26 articles.

1. Carbon, D. F. and Gingerich, O.: 1969, in O. Gingerich (ed.),Theory and Observation of Normal Stellar Atmospheres, MIT Press, Cambridge, p. 377.

2. Cester, B., Giurichin, G., Mardirossian, F., and Pucillo, M.: 1977,Astron. Astrophys. Suppl. 30, 223.

3. Fehrenbach, Ch., Duflot, M., Boulon, J., Rebeirot, E., and Lanoe, C.: 1966,Publ. Obs. de Haute Provence 8, 289.

4. Frank, F.: 1985,BAV Mitt., No. 36.

5. Giannone, P. and Giannuzzi, M. A.: 1974,Astrophys. Space Sci. 26, 289.

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1. 1SWASP J010313.78+352903.7: A Totally Eclipsing Binary with Components in Poor Thermal Contact;Research in Astronomy and Astrophysics;2022-12-09

2. HT Lyn and IR Lyn: Two Semi-detached-type Near-contact Binaries with Stable Orbital Period;Research in Astronomy and Astrophysics;2022-11-01

3. Evolution of Close Binary Systems;The Astrophysical Journal;2005-08-20

4. CN Andromedae: A Broken-Contact Binary?;The Astronomical Journal;2001-12

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