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Multipole Expansion Model in Gravitational Lensing

T. Fukuyama, Y. Kakigi, T. Okamura

astro-pharXiv:astro-ph/9702003

Abstract

Non-transparent models of multipole expansion model and two point-mass model are analyzed from the catastrophe theory. Singularity behaviours of 2n-pole moments are discussed. We apply these models to triple quasar PG1115+080 and compare with the typical transparent model, softened power law spheroids. Multipole expansion model gives the best fit among them.

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