Mc. Angoninwillaime et al., FURTHER OBSERVATIONAL EVIDENCE THAT MG J0414+0534 IS A GRAVITATIONAL MIRAGE, Astronomy and astrophysics, 281(2), 1994, pp. 388-394
Deep imaging of MG J0414+0534 with R and I filters reveals a faint, fu
zzy and red object at the exact location expected for a lensing galaxy
in the gravitational mirage hypothesis. Furthermore, the (extremely r
ed and almost featureless) spectra of the 2 brightest components are v
ery similar. These are strong indications that the system results from
multiple gravitational imaging of a single source, but the nature of
this source is not yet clear. It could be the nucleus of a low metalli
city galaxy at a high redshift or a new type of object. Significant di
fferences are observed between the flux ratios of the images at radio
and optical wavelengths. The most likely explanation for this effect i
s a differential amplification of the image pair A(1)-A(2) because of
the large magnification gradient near a caustic.