Since we see most binary systems from the side or inclined, the time-delay between the near and far points of the orbit smears out the signal making it harder to distinguish it from the noise.
因为我们看到的大部分双星系统都是从侧面或者倾斜的角度,轨道的近点和远地之间的时间差会干扰信号,使其更难从背景中分辨出来。
Since we see most binary systems from the side or inclined, the time-delay between the near and far points of the orbit smears out the signal making it harder to distinguish it from the noise.
因为我们看到的大部分双星系统都是从侧面或者倾斜的角度,轨道的近点和远地之间的时间差会干扰信号,使其更难从背景中分辨出来。
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