Abstract：We examine the stability of geometrically thin and opticallythick accretion disks to axisymmetric nearly radial perturbations.We derivea general dispersion relationship.These general results are applied for variousstandard disk models.Our results indicate that the axial component of wavevector of perturbation can lead to a new instability.
收稿日期: 1986-01-25
引用本文:
杨丕博,杨兰田,刘超. 薄吸积盘近径向扰动不稳定性[J]. , 1986, 25(1): 0-0.
杨丕博,杨兰田,刘超. ON THE INSTABILITY OF THIN ACCRETION DISKS TO NEARLY RADIAL PERTURBATION. , 1986, 25(1): 0-0.
