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首页> 外文期刊>The Astrophysical journal >On Synchronization in Detached Close Binaries: Reply to Rieutord and Zahn
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On Synchronization in Detached Close Binaries: Reply to Rieutord and Zahn

机译:关于分离式关闭二进制文件中的同步:回复Rieutord和Zahn

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In this paper we discuss the tidally driven meridional currents that spin down (or spin up) a nonsynchronous rotator in a time that is much shorter than the viscous decay time of residual motions. We refute the claim made by Rieutord & Zahn, who have argued that this large-scale meridional flow does not exist, so that the synchronization time should remain larger than the viscous time in a tidally distorted body. To be specific, they describe the internal motion by means of a series in the powers of the small parameter δ/R, which is the relative thickness of the Ekman boundary layer at the free surface.
机译:在本文中,我们讨论了潮汐驱动的子午电流,这些子午电流在比残余运动的粘性衰减时间短得多的时间内旋转(或旋转)非同步旋转器。我们驳斥了Rieutord&Zahn的说法,他们认为这种大规模的子午流不存在,因此同步时间应保持比在扭曲的物体中的粘性时间更长。具体来说,他们以小参数δ/ R的幂为单位来描述内部运动,该参数是自由表面上埃克曼边界层的相对厚度。

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