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: 11
ISSN: 0218-3013
eISSN: 1793-6608
Open Access Status: Green
DOI Link: https://doi.org/10.1142/S0218301318500933
Verlag: World Scientific Publishing
Abstract:
The evolution of close binary stars in mass asymmetry (transfer) coordinate is considered. The conditions for the formation of stable symmetric binary stars are analyzed. The role of symmetrization of asymmetric binary star in the transformation of potential energy into internal energy of star and the release of a large amount of energy is revealed.
Zitierstile
Harvard-Zitierstil: Sargsyan, V., Lenske, H., Adamian, G. and Antonenko, N. (2018) From dinuclear systems to close binary stars: Application to source of energy in the universe, International Journal of Modern Physics E, 27(11), Article 1850093. https://doi.org/10.1142/S0218301318500933
APA-Zitierstil: Sargsyan, V., Lenske, H., Adamian, G., & Antonenko, N. (2018). From dinuclear systems to close binary stars: Application to source of energy in the universe. International Journal of Modern Physics E. 27(11), Article 1850093. https://doi.org/10.1142/S0218301318500933
Schlagwörter
Close binary stars; mass asymmetry; mass transfer