Published June 1988 | Version v1
Journal article

High-resolution CCD imaging and derived gravitational lens models of 2237+0305

  • 1. Palomar Observatory, Pasadena, CA (USA)
  • 2. Haystack Observatory, Westford, MA (USA)
  • 3. Princeton Univ. Observatory, NJ (USA)
  • 4. Institute for Advanced Study, Princeton, NJ (USA)

Description

Images of the gravitational lens 2237+0305 acquired in good seeing have resolved the system into at least five components within the central few arsec of the object: the galaxy nucleus and four point sources in a ringlike formation approximately centered on the galaxy. It is found that the four point sources are distinctly bluer than the galaxy, but that they do not have identical colors. The observed configuration is well reproduced by a simple model that assumes that the four objects are images of the quasar and that the lens is a constant mass-to-light ratio, elliptical, de Vaucouleurs bulge. 29 references

Additional details

Publishing Information

Journal Title
Astron. J.
Journal Volume
95
Series
Astron. J.
Journal Page Range
1619-1628
ISSN
0004-6256
CODEN
ANJOA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
19102588
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
GALAXY CLUSTERS; GALAXY NUCLEI; GRAVITATIONAL LENSES; IMAGES; QUASARS; RED SHIFT
Descriptors DEC
COSMIC RADIO SOURCES; LENSES