Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...191...39k&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 191, no. 1, Feb. 1988, p. 39-43.
Astronomy and Astrophysics
Astrophysics
28
Digital Simulation, Galaxies, Gravitational Lenses, Imaging Techniques, Quasars
Scientific paper
Finding the positions, shapes and apparent brightnesses of images for given gravitational lens models is not a trivial task, since no global analytical inversion of the lens equation exists. The authors present here new numerical imaging procedures, which avoid the need for an inversion of the lens equation. The procedures are based on the principle of the conservation of surface brightness under gravitational deflection of light. The new imaging procedures lead to considerable simplifications in numerical simulations of deflector models for observed lens situations.
Kayser Rainer
Schramm Thomas
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