1146 + 111 B, C - A giant gravitational lens?

Physics – Optics

Scientific paper

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Astronomical Models, Gravitational Lenses, Quasars, Cosmology, Density Distribution, Galactic Structure, Geometrical Optics

Scientific paper

The quasars 1146 + 111 B, C have been claimed to be gravitationally lensed images of a single object. Lenses formed by a singular potential such as a string or black hole can be rejected because they would multiply image other quasars in the field. It is argued that a lensing potential well would have to be almost circularly symmetric and very soft. Furthermore, the observed overdensity of quasars in the field of 1146 + 111 B, C can be explained only if the counts of quasars at B over 22 mag exceed current estimates of a factor of more than 5. Elongated images of background galaxies tracing out the critical lines of the lens should be observable. Non-Gaussian density fluctuations would be necessary to reconcile the existence of a lens of this type with the smoothness of the microwave background. Unless independent evidence for these effects is forthcoming, the intepretation of this object as a gravitational lens is unlikely to be correct.

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