Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-26T10:44:44.970Z Has data issue: false hasContentIssue false
  • English
  • Français

An Interesting Pair of Active Galaxies

Published online by Cambridge University Press:  19 July 2016

X.-T. He ,
X.H. Xiao ,
S. Okamura ,
T. Noguchi ,
H. Maehara  and
R.D. Cannon
X.-T. He
Affiliation:
1. Department of astronomy, Peking Normal University, China
X.H. Xiao
Affiliation:
1. Department of astronomy, Peking Normal University, China
S. Okamura
Affiliation:
2. Tokyo Astronomical Observatory, University of Tokyo Mitaka, Tokyo 181, Japan
T. Noguchi
Affiliation:
2. Tokyo Astronomical Observatory, University of Tokyo Mitaka, Tokyo 181, Japan
H. Maehara
Affiliation:
2. Tokyo Astronomical Observatory, University of Tokyo Mitaka, Tokyo 181, Japan
R.D. Cannon
Affiliation:
3. Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ Scotland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A pair of emission-line galaxies with separation 7.1 arcseconds was found from the survey of the UK Schmidt objective-prizm plates. The spectroscopic observations by the 1.88m reflector of the Okayama Observatory show the same emission-line features with Z=0.0441.

Type
Chapter VIII: Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 124: Observational Cosmology , 1987 , pp. 531 - 534
Copyright
Copyright © Reidel 1987 

References

Baldwin, J., Phillips, M. and Terlevich, R. 1981, P.A.S.P., 93, 5.Google Scholar
Halpern, J., Marshall, H. and Oke, J. 1984, A.J., 89, 1802.Google Scholar
He, X.-T. and Impey, C. 1986, M.N.R.A.S., 221, 727.Google Scholar
Veron, M.-P. and Veron, P. 1985, ESO Scientific Report No.4.Google Scholar