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Researchers Reveal Rapid Mass Transfer between Twin Components in the Hierarchical Triple System
Author: | Update time:2021-06-09           | Print | Close | Text Size: A A A

In a study published in Monthly Notices of the Royal Astronomical Society, Dr. ZHAO Ergang and Prof. QIAN Shengbang from Yunnan Observatories of the Chinese Academy of Sciences revealed that rapid mass transfer between the two twin components in the eclipsing binary system GK Cepheus (hereafter GK Cep), which suggests that GK Cep is a key target to understand the mass transfer during binary evolution. And they also found that this system contains a solar-type stellar component expect the eclipsing binary.

GK Cep is an eclipsing binary that contains two A-type components with an orbital period of close to one day. Both two components are twins because of nearly the same mass, radius and effective temperature.

It is hard to observe total continuous light curve of GK Cep by using the ground-based telescope due to its unit period. The lunar-based ultraviolet telescope (hearafter LUT), a device in Chang’e 3 lunar lander, dedicated to continuously monitoring variable stars for as long as dozens of days in the near-ultraviolet band, which is not available on the ground.

The total continuous light curves are obtained with LUT and several eclipse times are monitored with the Sino-Thai 70-cm telescope of Lijiang Gaomeigu Station and the 1.0-m telescope in Yunnan observatories.

By analyzing the data of these light curves, the researchers revealed that GK Cep is a semi-detached system where the slightly less massive component is the hotter one filling its critical Roche lobe. The semi-detached configuration, together with the increase of the orbital period, suggests the mass transfer from secondary component to primary one, which could be proved by the hot spot found on the neck of the more massive by light curves. Combined with its high mass ratio, the researchers revealed that GK Cep is one of few close binaries on the key evolution state just after the shortest-period stage during rapidly mass transfer.

Apart from the continuous increase of the orbital period, the cyclic change could arise from the light-travel time effect of a solar-type stellar component, which is in good agreement with the third body contribution about 2.6% to the total light of the triple system from light curve. It could infer that the third body should have played an important role and the evolution of central binary could be accelerated during the interaction and the dynamical evolution.


ZHAO Ergang, Yunnan Observatories, CAS






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