galaxies;
fundamental parameters;
individual;
2237;
0305;
spiral;
gravitational lensing;
D O I:
10.1046/j.1365-8711.1998.01326.x
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
In the gravitational lens system Q2237 + 0305 the cruciform quasar image geometry is twisted by 10 degrees 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(-4)(+5). We measure a bar mass of (7.5 +/- 1.5) x 10(8) h(75)(-1) M. in the region inside the quasar images.