On the source of quasi-periodic oscillations of the black hole candidate GRS 1915+105: some new observations and their interpretation

A few classes of the light curve of the black hole candidate GRS 1915+105 have been analysed in detail. We discover that unlike the previous findings, quasi-periodic oscillations (QPOs) occasionally occur even in the so-called `On' or softer states. Such findings may require a revision of the accretion/wind scenario of the black hole candidates. We conjecture that considerable winds that are produced in `Off' states cool down as a result of Comptonization and fall back to the disc, creating an excess accretion rate and producing the so-called `On' state. After the drainage of the excess matter, the disc goes back to the `Off' state. Our findings strengthen the shock oscillation model for QPOs.