出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：We examine the evolution of the color radius and GRS 1915+105 and compare that to predictions
made by the Magnetic Flood Model. This model applies a linear correction to associate the Low
Frequency QPO to the Keplerian frequency. Because spectral fits to the X-ray data using XSpec
often produce erroneously low color radius results, the quantity is often ignored, but the trend is
assumed to be a valid trace of the inner disk radius. We show that, if the radius trend established by
the X-ray spectral fits can be believed, then no monotonic solution can rectify the QPO frequency
to the Keplerian radius. We discuss various caveats and analases that may be performed to further
test the Magnetic Flood model.
