The Oscillating state Sy1/NLSy1 Mkn110?

Details The Oscillating state Sy1/NLSy1 Mkn110? The Oscillating state Sy1/NLSy1 Mkn110?

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprb17083c&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

Mkn110 was observed three times by the Narrow Field Instruments onboard BeppoSAX. The broad band, 0.1-100 keV data, acquired 5 and 6 months apart, show marked spectral variations, anti-correlated with flux changes: the intrinsic power law continuum flattens as the source weakens. Mkn 100 is also known to vary in the optical band, both in the continuum and the intensity and width of the broad emission line. In analogy with the microquasar GRS 1915+105, we propose that the optical-to-X-ray spectral variations observed in this source are related to disk instabilities that develop at the border between the radiation pressure and the gas pressure dominated regions of an optically thick, geometrically thin, accretion disk. In this contribution we present our analysis and results.

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