We present observations of CLASS B2108+213, the widest separation
gravitational lens system discovered by the Cosmic Lens All-Sky Survey. Radio
imaging using the VLA at 8.46 GHz and MERLIN at 5 GHz shows two compact
components separated by 4.56 arcsec with a faint third component in between
which we believe is emission from a lensing galaxy. 5-GHz VLBA observations
reveal milliarcsecond-scale structure in the two lensed images that is
consistent with gravitational lensing. Optical emission from the two lensed
images and two lensing galaxies within the Einstein radius is detected in
Hubble Space Telescope imaging. Furthermore, an optical gravitational arc,
associated with the strongest lensed component, has been detected. Surrounding
the system are a number of faint galaxies which may help explain the wide image
separation. A plausible mass distribution model for CLASS B2108+213 is also
presented.Comment: 9 pages, 8 figures, accepted for publication in MNRA