Variability of the continuum emission of GQ Comae

Details Variability of the continuum emission of GQ Comae Variability of the continuum emission of GQ Comae

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296.1051s&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 1051-1052 (SEE N90-2

Astronomy and Astrophysics

Astronomy

Accretion Disks, Emission Spectra, Quasars, Thermal Radiation, Variability, Active Galactic Nuclei, Astronomical Models, Galactic Radiation, Light (Visible Radiation), Ultraviolet Radiation

Scientific paper

The optical/UV part of the spectrum of GQ Comae (1202+281) is analyzed. It is accepted that the optical/UV/soft X-ray big bump in Active Galactic Nuclei (AGN) spectra is caused by the thermal radiation from an accretion disc. Attributing the observed variability in AGN spectra to the accretion disc instabilities, both the continuum shape and variability of GQ Comae can be explained. Constraints on some model parameters are established.

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