PARAMETER DEGENERACY IN MODELS OF THE QUADRUPLE LENS SYSTEM Q2237+0305

被引:103
作者
WAMBSGANSS, J [1 ]
PACZYNSKI, B [1 ]
机构
[1] PRINCETON UNIV OBSERV,PRINCETON,NJ 08544
关键词
D O I
10.1086/117144
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The geometry of the quadruple lens system Q2237+0305 is modeled with a simple astigmatic lens: a power-law mass distribution: m similar to r(beta) with an external shear gamma. The image positions can be reproduced with an accuracy better than 0.01 arcsec for any 0.0 less than or equal to beta less than or equal to 1.85 and the corresponding value of gamma=0.1385-0.0689 beta. This is a factor of similar to 4 more precise than what can be achieved by the best constant M/L lens models [Rix et al., AT, 104, 959 (1992)]. The image intensity ratios and the time delay ratios are almost constant along our one parameter family of models, but the total magnification varies from 8 to >1000, and the maximum time delay (between leading image B and trailing image C) for H-0 of 75 km s(-1) Mpc(-1) varies from more than 20 h to about 1.5 h, while beta increases from 0.0 to 1.85.
引用
收藏
页码:1156 / 1162
页数:7
相关论文
共 23 条
[11]   GRAVITATIONAL MICROLENSING AT LARGE OPTICAL DEPTH [J].
PACZYNSKI, B .
ASTROPHYSICAL JOURNAL, 1986, 301 (02) :503-516
[12]  
PEN U, 1993, 31ST P LIEG INT ASTR, P11
[13]  
Press W. H., 1992, NUMERICAL RECIPES EX
[14]   5TH IMAGE AND PHOTOMETRIC VARIABILITY IN 2237+0305 (EINSTEIN CROSS) [J].
RACINE, R .
ASTRONOMICAL JOURNAL, 1991, 102 (02) :454-460
[15]   MICROLENSING AND THE STRUCTURE OF ACTIVE GALACTIC NUCLEUS ACCRETION DISKS [J].
RAUCH, KP ;
BLANDFORD, RD .
ASTROPHYSICAL JOURNAL, 1991, 381 (02) :L39-L42
[16]  
RIX HW, 1988, AJ, V95, P1619
[17]  
RIX HW, 1988, AJ, V96, P1755
[18]  
Schneider P., 1992, GRAVITATIONAL LENSES
[19]  
Tyson T., 1985, Sky and Telescope, V70, P319
[20]  
WAMBSGANSS J, 1990, MPA550 MAX PL REP