Journalartikel
Autorenliste: Sargsyan, V. V.; Lenske, H.; Adamian, G. G.; Antonenko, N. V.
Jahr der Veröffentlichung: 2018
Zeitschrift: International Journal of Modern Physics E
Bandnummer: 27
Heftnummer: 7
ISSN: 0218-3013
eISSN: 1793-6608
DOI Link: https://doi.org/10.1142/S0218301318500635
Verlag: World Scientific Publishing
Abstract:
Applying the microscopic nuclear physics ideas to macroscopic stellar systems, we study the evolution of the compact di-stars in mass asymmetry (transfer) coordinate. Depending on the internal structure of constituent stars, the initial mass asymmetry, total mass, and orbital angular momentum, the close di-star system can either exist in symmetric configuration or fuse into mono-star. The limitations for the formation of stable symmetric binary stars are analyzed.
Zitierstile
Harvard-Zitierstil: Sargsyan, V., Lenske, H., Adamian, G. and Antonenko, N. (2018) From dinuclear systems to close binary stars: Application to mass transfer, International Journal of Modern Physics E, 27(7), Article 1850063. https://doi.org/10.1142/S0218301318500635
APA-Zitierstil: Sargsyan, V., Lenske, H., Adamian, G., & Antonenko, N. (2018). From dinuclear systems to close binary stars: Application to mass transfer. International Journal of Modern Physics E. 27(7), Article 1850063. https://doi.org/10.1142/S0218301318500635
Schlagwörter
Close di-star system; mass asymmetry; mass transfer
