Images for a Binary Gravitational Lens from a Single Real Algebraic Equation
arXiv:astro-ph/0206267 · doi:10.1051/0004-6361:20020891
Abstract
It is shown that the lens equation for a binary gravitational lens being a set of two coupled real fifth-order algebraic equations (equivalent to a single complex equation of the same order) can be reduced to a single real fifth-order algebraic equation, which provides a much simpler way to study lensing by binary objects.
4 pages; accepted for publication in A&A Letters
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- Strong Lensing by Binary Galaxies Modelled as Isothermal Spheres
- Images for an Isothermal Ellipsoidal Gravitational Lens from a Single Real Algebraic Equation
- Euclidean Algorithm for a Gravitational Lens in a Polynomial Equation
- Perturbation theory of N point-mass gravitational lens systems without symmetry: small mass-ratio approximation
- An optical n-body gravitational lens analogy
- Effects of a deformation of a star on the gravitational lensing
- Evolutionary algorithm-based analysis of gravitational microlensing lightcurves
- Effects of the core radius of an isothermal ellipsoidal gravitational lens on the caustics and the critical curves