论文标题
RR Lyncis的日食时间
The eclipse timings of RR Lyncis
论文作者
论文摘要
重新调查了明亮的，怪异的二进制RR Lyncis的最小时代。从苔丝的数据中可以发现，日食时机（尤其是对于初级最小值）的显着差异可能是由于脉动引起的日食剖面的较小，不规则变化所致，而不是光曲线不对称。
The times of minima of the bright, eccentric eclipsing binary RR Lyncis are re-investigated. From the TESS data it is found that significant differences in the eclipse timings, particularly for the primary minima, are probably due to small, irregular changes in the eclipse profile due to pulsations, rather than light-curve asymmetries.
