A method to map quasar flares via gravitational lensing

Details A method to map quasar flares via gravitational lensing A method to map quasar flares via gravitational lensing

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004an....325..258y&link_type=abstract

Astronomische Nachrichten, Vol.325, Issue 3, p.258-258

Astronomy and Astrophysics

Astronomy

Scientific paper

Quasars exhibit stochastic non-periodic flux variations that can be
observed in various wavebands. These variations are believed to
originate from instabilities in quasar accretion disks, but we cannot
directly confirm this from current observations due to the extremely
small angular size, ˜ 1 μ as.

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