PROPAGATION OF TIDAL DISTURBANCE IN GASEOUS ACCRETION DISKS

被引：33

作者：

LIN, DNC

PAPALOIZOU, JCB

SAVONIJE, GJ

机构：

[1] QUEEN MARY & WESTFIELD COLL,SCH MATH SCI,LONDON E1 4NS,ENGLAND

[2] UNIV AMSTERDAM,INST ASTRON,1018 WB AMSTERDAM,NETHERLANDS

来源：

ASTROPHYSICAL JOURNAL | 1990年 / 365卷 / 02期

关键词：

Hydrodynamics; Planets: formation; Stars: accretion; Stars: binaries;

D O I：

10.1086/169528

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We continue our investigation on linear wave propagation in geometrically thin accretion disks where the equilibrium variables, such as density and temperature, are stratified in the direction normal to the plane of the disk, i.e., the vertical direction. We show, due to refraction effects, that waves excited by tidal disturbances induced by a satellite or a companion of the central object are not expected to reach the interior regions of the disk with a significant amplitude.

引用

页码：748 / 756

页数：9

共 21 条

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