Published July 1988
| Version v1
Journal article
1343.4+2640 - a close quasar pair
Creators
- 1. Ohio State Univ., Columbus (USA)
- 2. British Columbia Univ., Vancouver (Canada)
- 3. Arizona State Univ., Tempe (USA)
- 4. Dominion Astrophysical Observatory, Victoria (Canada)
Description
Two quasars of virtually identical redshift separated by 9.5 arcsec have been discovered on a CFHT grens plate. Subsequent spectroscopy reveals substantial differences in their spectral line strengths which appear to be incompatible with a gravitational lens hypothesis. Furthermore, deep CCD images of the field do not show any indication of a lensing galaxy or extended Ly-alpha emission. It is likely that these quasars are a physically related pair, possibly residing in a cluster of galaxies at z = 2.03. 13 references
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 330
- Series
- Astrophys. J.
- Journal Page Range
- 184-190
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20000905
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; COORDINATES; COSMOLOGY; GALAXY CLUSTERS; GRAVITATIONAL LENSES; LYMAN LINES; QUASARS; RED SHIFT; SPECTROSCOPY
- Descriptors DEC
- COSMIC RADIO SOURCES; LENSES; STARS