HST observations and models of the gravitational lens system MG 0414+0534

被引:58
作者
Falco, EE
Lehar, J
Shapiro, II
机构
[1] Harvard-Smithsonian Ctr. Astrophys., Cambridge, MA 02138
关键词
D O I
10.1086/118274
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Quadruple gravitational lens systems offer the possibility of measuring time delays for image pairs, microlensing effects, and extinction in distant galaxies. Observations of these systems may be used to obtain estimates of Ho and to study the various mass components of lens galaxies at high redshifts. With the Hubble Space Telescope, we have observed the reddest known gravitational lens system, MG 0414+0534. We used WFPC2/PC1 to obtain deep, high-resolution images with two filters, F675W and F814W. We present a detailed analysis of all of the components of MG 0414, as well as macrolens models. Our main results are: (1) confirmation that MG 0414 is inescapably a gravitational lens system; (2) discovery of a blue are connecting the 3 brightest images of the QSO central core; (3) accurate positions and apparent brightnesses for all 4 known images of the QSO central core and for the lens galaxy G; (4) a good representation of the brightness distribution of G by elliptical isophotes with a De Vaucouleurs profile, characteristic of an elliptical galaxy; (5) models that consist of simple elliptical potentials and account qualitatively, but not quantitatively, for the HST image positions, are morphology and radio flux ratios for the images of the QSO central core; (6) a possible new test to distinguish between reddening in the host galaxy of the QSO and in the lens galaxy, based on future accurate measurements of spatial variations in the color of the are; and (7) the suggestion that microlensing is a plausible cause for the differences between the radio and optical flux ratios for the brightest images, A1 and A2. Further observations and measurements such as of the redshift of the lens galaxy, can be used fruitfully to study microlensing for this system. (C) 1997 American Astronomical Society.
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页码:540 / 549
页数:10
相关论文
共 25 条
[1]  
ANGONINWILLAIME MC, 1994, ASTRON ASTROPHYS, V281, P388
[2]   GRAVITATIONAL IMAGING BY ISOLATED ELLIPTIC POTENTIAL WELLS .1. CROSS-SECTIONS [J].
BLANDFORD, RD ;
KOCHANEK, CS .
ASTROPHYSICAL JOURNAL, 1987, 321 (02) :658-675
[3]   Visibility LensClean and the reliability of deconvolved radio images [J].
Ellithorpe, JD ;
Kochanek, CS ;
Hewitt, JN .
ASTROPHYSICAL JOURNAL, 1996, 464 (02) :556-567
[4]   VLA observations of the gravitational lens system Q2237+0305 [J].
Falco, EE ;
Lehar, J ;
Perley, RA ;
Wambsganss, J ;
Gorenstein, MV .
ASTRONOMICAL JOURNAL, 1996, 112 (03) :897-901
[5]  
FALCO EE, 1993, P 31 LIEG INT C, P127
[6]  
HEWITT J, 1989, LECT NOTES PHYSICS, V390
[7]   A GRAVITATIONAL LENS CANDIDATE WITH AN UNUSUALLY RED OPTICAL COUNTERPART [J].
HEWITT, JN ;
TURNER, EL ;
LAWRENCE, CR ;
SCHNEIDER, DP ;
BRODY, JP .
ASTRONOMICAL JOURNAL, 1992, 104 (03) :968-979
[8]  
HOLTZMAN JA, 1996, IN PRESS PASP
[9]  
KATZ CA, 1993, APJ, V409, P9
[10]   DO THE REDSHIFTS OF GRAVITATIONAL LENS GALAXIES RULE OUT A LARGE COSMOLOGICAL CONSTANT [J].
KOCHANEK, CS .
ASTROPHYSICAL JOURNAL, 1992, 384 (01) :1-11