Publication Date:
2013-08-29
Description:
Preliminary results of a multifrequency monitoring campaign for the bright, Seyfert 1 galactic nuclei Mkn335 are presented. Nearly uniform sampling at 3 day intervals is achieved quasi simultaneously at each wavelength band. Wavelength dependent variability is seen at the 20 to 30 percent level. Interpretation of variability in terms of geometrically thin, optically thick accretion disk models is discussed. The inferred blackhole masses and accretion rates are discussed. Possible correlation between continuum and emission line variations is discussed.
Keywords:
ASTROPHYSICS
Type:
ESA, Evolution in Astrophysics: IUE Astronomy in the Era of New Space Missions; p 557-559
Format:
text
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