Mass and Spin of GRS 1915+105 Based on a Resonance Model of QPOs
arXiv:astro-ph/0407251 · doi:10.1093/pasj/56.5.L25
Abstract
We demonstrate that the four high-frequency QPOs observed in GRS 1915+105 can be interpreted as the oscillation modes on disks which non-linearly and resonantly interact with a warp. The warp is assumed to be a low-frequency global pattern on the disk. This identification suggests that the relevant mass, , and spin, , of GRS 1915+105 are, and
4 pages, 5 figures, accepted in PASJ Vol.56(2004) No.5, The English was improved on September 1
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