PMN J0134-0931: A gravitationally lensed quasar with an unusual radio morphology
Joshua N. Winn, James E. J. Lovell, Hsiao-Wen Chen, Andre B. Fletcher, Jacqueline N. Hewitt, Alok R. Patnaik, Paul L. Schechter
Abstract
The radio-loud quasar PMN J0134-0931 was discovered to have an unusual morphology during our search for gravitational lenses. In VLA and MERLIN images, there are 5 compact components with maximum separation 681 millarcseconds. All of these components have the same spectral index from 5 GHz to 43 GHz. In a VLBA image at 1.7 GHz, a curved arc of extended emission joins two of the components in a manner suggestive of gravitational lensing. At least two of the radio components have near-infrared counterparts. We argue that this evidence implies that J0134-0931 is a gravitational lens, although we have not been able to devise a plausible model for the foreground gravitational potential. Like several other radio-loud lenses, the background source has an extraordinarily red optical counterpart.
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