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Article
Affiliation(s)

Department of Physics, Jiangxi Normal University, Nanchang 330000, China

ABSTRACT

 The formation and evolution of binary stars are key steps in star formation and evolution, and thus their research has become the core content of modern astronomical research. Although as early as 1976, Bodan Pachenski proposed the theory of the evolution of shared envelopes in binary stars, but it was never confirmed until 2022 when the Yunnan Astronomical Observatory of the Chinese Academy of Sciences and an Australian team first observed the phenomenon of shared envelope ejection in binary stars, which provided support for Bodan Pachenski’s theory, but the true formation mechanism and evolution process of binary stars remain undetermined. For this reason, the author of this paper has proposed a theory of the formation and evolution of binary stars based on the theory of the evolution of common envelopes in binary stars and the theory of tidal disruption events, laying a foundation for establishing a complete theory of star formation and evolution.

KEYWORDS

Binary star common envelope evolution theory, binary star common envelope ejection phenomenon, tidal disruption, evolution of binary star.

Cite this paper

Cui-xiang Zhong.Formation and Evolution of Binary Stars in the Cosmic Environment.Journal of Environmental Science and Engineering B 15 (2026) 42-54

References
[1] Taam, R. E., and Sandquist, E. L. 2000. “Common Envelope Evolution of Massive Binary Stars.” Annual Review of Astronomy and Astrophysics 38: 113-41.
[2] Li, J.-J., Xiong, J.-P., Tian, Z.-J., Liu, C., Han, Z. W., and Chen, X.-F. 2025. “Identify Main-Sequence Binaries from the Chinese Space Station Telescope Survey with Machine Learning. II. Based on Gaia and GALEX.” The Astronomical Journal 169: 220.
[3] Hurley, J. R., Tout, C. A., and Pols, O. R. 2000. “Evolution of Binary Stars and the Effect of Tides on Binary Populations.” Mon. Not. R. Astron. Soc. 000: 1-36.
[4] Pollack, J. B., Hubickyj, O., Bodenheimer, P., Lissauer, J. J., Podolak, M., and Greenzweig, Y. 1996. “Formation of the Giant Planets by Concurrent Accretion of Solids and Gas.” Icarus 124: 62-85.
[5] Popper, D. M. 1978. “Masses of Hot Main-Sequence Stars.” Astrophysical Journal 220: L11-L14.
[6] Laughlin, G., Bodenheimer, P., and Adams, F. C. 1997. “The End of the Main Sequence.” The Astrophysical Journal 482: 420.
[7] Sollerman, J., Taddia, F., Arcavi, I., Fremling, C., Fransson, C., Burke, J., Cenko, S. B., Andersen, O., Andreoni, I., Barbarino, C., Blagorodova, N., Brink, T. G., Filippenko, A. V., Gal-Yam, A., Hiramatsu, D., Hosseinzadeh, G., Howell, D. A., de Jaeger, T., Lunnan, R., McCully, C., Perley, D. A., Tartaglia, L., Terreran, G., Valenti, S., and Wang, X. 2019. “Late-Time Observations of the Extraordinary Type II Supernova iPTF14hls.” Astronomy and Astrophysics 621: A30.
[8] Tauris, T. 2014. “Neutron Star Formation and Evolution—Singles, Binaries and Triples.” 40th COSPAR Scientific Assembly, held 2-10 August 2014, in Moscow, Russia.
[9] Haehnelt, M. G., and Kauffmann, G. 2001. The Formation and Evolution of Supermassive Black Holes and Their Host Galaxies. Berlin Heidelberg: Springer, 364-74.
[10] Wu, X. B., Wang, F. G., Fan, X. H., Yi, W. M., Zuo, W. W., Bian, F. Y., Jiang, L. H., McGreer, I. D., Wang, R., Yang, J. Y., Yang, Q., Thompson, D., and Beletsky, Y. 2015. “An Ultra Luminous Quasar with a Twelve-Billion-Solar-Mass Black Hole at Red Shift 6.30.” Nature 518 (7540): 512-5.

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