Spectral microvariability in Quasars

Details Spectral microvariability in Quasars Spectral microvariability in Quasars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..32...46r&link_type=abstract

The Nuclear Region, Host Galaxy and Environment of Active Galaxies (Eds. Erika Benítez, Irene Cruz-González, & Yair Krongold) Re

Astronomy and Astrophysics

Astronomy

Accretion, Accretion Disks, Galaxies: Active, Quasars: Emission Lines

Scientific paper

Optical microvariability (OM, small amplitude variations in time scales
from minutes to hours) in radio-quiet quasars (RQQ) may be as frequent
as in radio-loud quasars (RLQ) (de Diego et al. 1998; Ramírez et
al. 2007). However, observations cannot still establish the origin of
OM.

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