Rayleigh-Taylor instability of two viscous superposed rotating and conducting fluids |
| |
| Authors: | P K Bhatia R P S Chhonkar |
| |
| Institution: | (1) Observatorio Astronómico de Córdoba and IMAF, Universidad Nacional, Córdoba, Argentina;(2) Observatorio Astronómico de Córdoba, Universidad Nacional, Córdoba, Argentina |
| |
| Abstract: | Classical R-M and synthetic W-D analysis of V758 Centauri are presented. Two solutions (semi-detached and contact) were found from differential corrections approach. The semi-detached model is physically acceptable since the system is thermally decoupled. The solution for this case and the photometric data are consistent with a B9 primary and A9 secondary components having parameters close to Main-Sequence values. It is suggested that V758 Centauri is a B-type W UMa system at the brokencontact phase predicted by the Thermal Relaxation Oscillations theory. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
