Variability in BL Lac objects: A schematic model

Details Variability in BL Lac objects: A schematic model Variability in BL Lac objects: A schematic model

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..825m&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 2: AGN and the X Ray Background p 825-829 (SEE N90-258

Astronomy and Astrophysics

Astronomy

6

Bl Lacertae Objects, Shock Waves, Stellar Models, Variability, Frequencies, Relativistic Velocity, Stellar Interiors, Stellar Magnetic Fields, Ultraviolet Radiation, X Ray Spectra

Scientific paper

The systematic variability properties of BL Lac objects at ultraviolet and X-ray frequencies are considered. A theoretical model, based on the propagation of a perturbation along a relativistic jet can account for the observed spectral hardening with increasing intensity in the X-ray band. The observed variability amplitude is predicted to depend on the angle of view.

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