The C [CLC][CSC]iv[/CSC][/CLC] Absorption–M[CLC]g[/CLC] [CLC][CSC]ii[/CSC][/CLC] Kinematics Connection in 〈[CLC][ITAL]z[/ITAL][/CLC]〉 ∼ 0.7 Galaxies
The Astrophysical Journal1999Vol. 519(1), pp. L43–L46
Citations Over TimeTop 10% of 1999 papers
Christopher W. Churchill, Richard R. Mellon, J. C. Charlton, Buell T. Jannuzi, Sofia Kirhakos, Charles C. Steidel, Donald P. Schneider
Abstract
We have examined Faint Object Spectrograph data from the Hubble Space Telescope Archive for CIV 1548,1550 absorption associated with 40 MgII 2796,2803 absorption-selected galaxies at 0.4 color; if further data corroborate this trend, in view of the strong CIV-MgII kinematics correlation, it could imply a connection between stellar populations, star formation episodes, and the kinematics and ionization conditions of halo gas at z~1.