Published June 1988
| Version v1
Journal article
High-resolution CCD imaging and derived gravitational lens models of 2237+0305
Creators
- 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