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The Light Curve and the Orbital Period Variations of Binary System TT Andromedae
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作者 davood manzoori Salar Abbasvand Vahid Abbasvand 《International Journal of Astronomy and Astrophysics》 2017年第2期112-123,共12页
The first photoelectric light curve analysis of the TT And system in a broad band filter (400 - 700 nm) was carried out using the PHOEBE program. The absolute dimensions of the system are determined and its evolution ... The first photoelectric light curve analysis of the TT And system in a broad band filter (400 - 700 nm) was carried out using the PHOEBE program. The absolute dimensions of the system are determined and its evolution is discussed. The most distinct feature of the system is a comparatively very low mass of the cooler component i.e. M2 = 0.26M⊙. Moreover, using the Observed-minus-Calculated data, the period changes of the system are studied, which reveal the presence of a third body orbiting the system with a period P3 = 63.89 yr, superimposed on which is a secular period increase, which is ascribed to mass transfer with a rate &minus;7.60 × 10&minus;12 M⊙ yr&minus;1 from the cooler secondary component. 展开更多
关键词 Binaries: ECLIPSING Stars: Evolution Stars: Individual (TT And)
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