Pseudo elliptical lensing mass model: Application to the NFW mass distribution

被引:111
|
作者
Golse, G [1 ]
Kneib, JP [1 ]
机构
[1] Observ Midi Pyrenees, Astrophys Lab, F-31400 Toulouse, France
关键词
cosmology : miscellaneous; gravitational lensing; dark matter; galaxies : clusters : general; galaxies : halos;
D O I
10.1051/0004-6361:20020639
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We introduce analytical expressions for a pseudo fully analytical elliptical projected Navarro, Frenk & White (NFW) mass profile to be used in lensing equations. We propose a formalism that incorporates the ellipticity into the expression for the lens potential, producing a pseudo-elliptical mass distribution. This approach can be implemented to any circular mass profile for which the projected mass profile Sigma(r) and the deflection angle profile alpha(r) both have analytical expressions; however the potential does not necessarily need to take an analytical form. We apply this new formalism to the NFW mass distribution and study how well this pseudo-elliptical NFW model describes an elliptical mass distribution. We conclude that the pseudoelliptical NFW model is a good description of elliptical mass distributions provided that the ellipticity of the projected mass distribution is less than or similar to 0.4, although with a slightly boxy distribution.
引用
收藏
页码:821 / 827
页数:7
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