High-redshift superwinds as the source of the strongest Mg II absorbers: A feasibility analysis

Astrophysical Journal

Volumn 562, Issue 2 PART II, 2001, Pages 641-648

  Bond, Nicholas A ^a   Churchill, Christopher W ^a   Charlton, Jane C ^a   Vogt, Steven S ^b  

^a PENNSYLVANIA STATE UNIVERSITY   (United States)

^b University of California at Santa Cruz   (United States)

Author keywords

Galaxies: High redshift; Galaxies: Ism; Ism: Bubbles; Quasars: Absorption lines

Indexed keywords

EID: 0042755646     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/323876     Document Type: Article

References (6)

1. Adelberger, K. L., Steidel, C. C., Giavalisco, M., Dickinson, M., Pettini, M., & Kellogg, M. 1998, ApJ, 505, 18
2. Bechtold, J., Green, R. F., & York, D. G. 1987, ApJ, 312, 50
3. Charlton, J. C., & Churchill, C. W. 1998, ApJ, 499, 181
4. Churchill, C. W. 1997, Ph.D. thesis, Univ, California, Santa Cruz
5. 1999, in ASP Conf. Ser. 200, Clustering at High Redshift, ed. A. Mazure, O. Le Fèvre, & V. Le Brun (San Francisco: ASP), 271
6. 2001, ApJ, 560, 92