| Title: |
Origin of the orbital period change in contact binary stars |
| Authors: |
Sargsyan, V. V., Lenske, H., Adamian, G. G., Antonenko, N. V. |
| Publication Year: |
2019 |
| Collection: |
Astrophysics |
| Subject Terms: |
Astrophysics - Solar and Stellar Astrophysics |
| More Details: |
The evolution of contact binary star systems in mass asymmetry (transfer) coordinate is considered. The orbital period changes is explained by an evolution in mass asymmetry towards the symmetry (symmetrization of binary system). It is predicted that a decreasing and an increasing orbital periods are related, respectively, with the non-overlapping and overlapping stage of the binary star during its symmetrization. A huge amount of energy $\Delta U\approx 10^{41}$ J is converted from the potential energy into internal energy of the stars during the symmetrization. As shown, the merger of stars in the binary systems, including KIC 9832227, is energetically an unfavorable process. The sensitivity of the calculated results to the values of total mass and orbital angular momentum is analyzed.
Comment: 14 pages, 24 figures. The article accepted to IJMPE. arXiv admin note: substantial text overlap with arXiv:1812.11338 |
| Document Type: |
Working Paper |
| DOI: |
10.1142/S0218301319500447 |
| Access URL: |
http://arxiv.org/abs/1907.02820 |
| Accession Number: |
edsarx.1907.02820 |
| Database: |
arXiv |
