National Radio Astronomy Observatory
P.O. Box O
Socorro, NM 87801
http://www.nrao.edu
April 3, 2003
Contact:
Dave Finley, Public Information Officer
Socorro, NM
(505) 835-7302
dfinley@nrao.edu
Artist's conception of the disk of star-forming
gas around the center of the galaxy hosting the
quasar PSS J2322+1944. The disk is about
13,000 light-years in diameter. The luminous
quasar, powered by the infall of matter into a
supermassive black hole, is at the center.
(Click on Image for Larger Version)
Credit: Geraint Lewis, University of Sydney,
NRAO/AUI/NSF
Optical (visible-light) image of quasar
PSS J2322+1944, made at the W.M. Keck Observatory,
showing twin images indicating gravitational
lensing (left). At right, a VLA image showing
redshifted CO gas emission, revealing the
"Einstein Ring" lens effect. The crosses in
this image indicate locations of the optical
quasar images.
(Click on Image for Larger Version)
Credit: G. Djorgovski; C. Carilli et al., NRAO/AUI/NSF
The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.