Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-19T08:32:25.328Z Has data issue: false hasContentIssue false

Galaxy Evolution from QSO Absorption-Line Selected Samples

Published online by Cambridge University Press:  25 May 2016

Mark Dickinson
Affiliation:
STScI, 3700 San Martin Dr., Baltimore MD 21218, USA
Charles C. Steidel
Affiliation:
Caltech Astronomy, MS 105-24, Pasadena CA 91125, USA

Extract

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.

Although a connection between certain classes of QSO absorption line systems and gas associated with galaxies was hypothesized long ago, the first systematic evidence supporting this was provided by Bergeron & Boissé (1991). Observing QSOs with known Mgll absorption lines at zabs < zQSO, they identified galaxies near the QSO sightline and spectroscopically confirmed that their redshifts matched those of the MgII absorption doublet.

Type
Galaxies in Formation
Copyright
Copyright © Kluwer 1996 

References

Bergeron, J., and Boissé, P. 1991, A&A, 243, 344.Google Scholar
Cowie, L.L., Hu, E.M., and Songaila, A. 1995, Nature, 377, 603.Google Scholar
Lilly, S.J., Tresse, L., Hammer, F., Crampton, D., and Le Fèvre, O. 1995, ApJ. (in press).Google Scholar
Steidel, C.C., and Dickinson, M. 1992, ApJ., 394, 81.Google Scholar
Steidel, C.C., Dickinson, M., and Persson, S.E. 1994, ApJ., 437, L75.Google Scholar
Steidel, C.C., and Dickinson, M. 1995, in Wide Field Spectroscopy & the Distant Universe, eds. Maddox, S. and Aragón–Salamanca, A., World Scientific, p. 349.Google Scholar
Steidel, C.C., in QSO Absorption Lines, ed. Meylan, G., Springer, p. 139.Google Scholar