DISK MODELS FOR MCG-06-30-15 - THE VARIABILITY CHALLENGE

Recent observations have shown that the Fe K alpha line profile of the Seyfert 1 galaxy MCG -06-30-15 is strongly variable. We attempt accre tion disk model fits to the Fe K alpha Line profiles in high, low, and medium continuum luminosity phases of this source. During the monitor ing by Iwasawa et al., a broad redshifted component remained reasonabl y constant, while a narrower component at approximate to 6.4 keV respo nded strongly to continuum changes. Physically consistent fits are pos sible if the index xi of the power-law emissivity changes from 0.7 (hi gh phase) to 3.0 (low phase). The shape of the redshifted component at the low phase is crucial to the disk model interpretation. We suggest that the actual shape may be a broad redshifted Gaussian. Three lines of evidence support the interpretation of the Fe K alpha line as cons isting of multiple components, beyond the lack of correlation in the r esponse to continuum changes of the red and blue components in MCG -06 -30-15: (1) We show that the strong concentration of narrow-peak centr oids at 6.4 keV is inconsistent with expectations of a random distribu tion of disk orientations. (2) The average Fe K alpha profile for a sa mple of 16 mostly Seyfert 1 galaxies suggests a natural decomposition into two Gaussians: one is unshifted/narrow, and the other is redshift ed/broad. (3) Evidence for emission in excess of the expectation of di sk models on the high-energy side of the Fe K alpha profile is both a challenge for low-inclination disk models and support for the two-comp onent decomposition.