The time delays of gravitational lens HE 0435-1223: An early-type galaxy with a rising rotation curve

被引:136
作者
Kochanek, CS
Morgan, ND
Falco, EE
McLeod, BA
Winn, JN
Dembicky, J
Ketzeback, B
机构
[1] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[3] Apache Point Observ, Sunspot, NM 88349 USA
关键词
cosmological parameters; dark matter; galaxies : kinematics and dynamics; gravitational lensing; quasars : individual (HE 0435-1223);
D O I
10.1086/499766
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
`We present Hubble Space Telescope images and 2 years of optical photometry of the quadruple quasar HE 0435-1223. The time delays between the intrinsic quasar variations are Delta t(AD) = -14.37(-0.85)(+0.75), Delta t(AB)= -8.00(-0.82)(+0.73), and Delta t(AC) = 2.10(-0.71)(+0.78) days. We also observed nonintrinsic variations of similar to 0.1 mag yr(-1) that we attribute to microlensing. Instead of the traditional approach of assuming a rotation curve for the lens galaxy and then deriving the Hubble constant (H-0), we assume H-0 ( 72 +/- 7) km s(-1) Mpc(-1) and derive constraints on the rotation curve. On the scale over which the lensed images occur (1."2 = 5 h(-1) kpc similar or equal to 1.5R(e)), the lens galaxy must have a rising rotation curve, and it cannot have a constant mass- to- light ratio. These results add to the evidence that the structures of earlytype galaxies are heterogeneous.
引用
收藏
页码:47 / 61
页数:15
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