Strong gravitational lensing and galactic bulges

Details Strong gravitational lensing and galactic bulges Strong gravitational lensing and galactic bulges

2003-01-03

arxiv.org/abs/astro-ph/0301037v2

Astrophys.J. 587 (2003) L55-L58

Astronomy and Astrophysics

Astrophysics

13 pages, 2 figures, the shortened version was accepted by ApJ(Letters)

Scientific paper

10.1086/375180

Lensing probabilities of quasars with image separations greater than \Delta\theta and flux density ratios less than q_{\mathrm{r}} are calculated by foreground dark matter halos in a flat, cosmological constant dominated (\LambdaCDM) universe . The mass density of the lenses is taken to be the Navarro-Frenk-White (NFW) profile on all mass scales, plus a central point mass for low-mass halos with M

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