Abstract
We present the results from VLBI observations at three frequencies of the gravitational lens system B0218+357. From the source double structure, seen in both the A and B images at 15 GHz, we have derived a relative magnification matrix, and we show that the lens mass distribution must be non-spherical. We investigate how far the matrix parameters derived from 15 GHz observations can be used to relate the A and B images at 1.7 and 5 GHz, where the image sizes are much larger.
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© 1996 International Astronomical Union
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Porcas, R.W., Patnaik, A.R. (1996). Multi-Frequency VLBI Observations of B0218+357. In: Kochanek, C.S., Hewitt, J.N. (eds) Astrophysical Applications of Gravitational Lensing. International Astronomical Union / Union Astronomique Internationale, vol 173. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0221-3_89
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DOI: https://doi.org/10.1007/978-94-009-0221-3_89
Publisher Name: Springer, Dordrecht
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