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RobertSchmidt Rachel L.Webster Geraint F.Lewis 《Monthly notices of the Royal Astronomical Society》1998,295(2):488-496
In the gravitational lens system Q2237+0305 the cruciform quasar image geometry is twisted by 10c by the lens effect of a bar in the lensing galaxy. This effect can be used to measure the mass of the bar. We construct a new lensing model for this system with a power-law elliptical bulge and a Ferrers bar. The observed ellipticity of the optical isophotes of the galaxy leads to a nearly isothermal elliptical profile for the bulge, with a total quasar magnification of 16+5 −4 . We measure a bar mass of (7.5 ∼ 1.5) −108 h −1 75 M⊙ in the region inside the quasar images. 相似文献
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