Authors:
Murphy, MT
Webb, JK
Flambaum, VV
Dzuba, VA
Churchill, CW
Prochaska, JX
Barrow, JD
Wolfe, AM
Citation: Mt. Murphy et al., Possible evidence for a variable fine-structure constant from QSO absorption lines: motivations, analysis and results, M NOT R AST, 327(4), 2001, pp. 1208-1222
Citation: Mt. Murphy et al., Possible evidence for a variable fine-structure constant from QSO absorption lines: systematic errors, M NOT R AST, 327(4), 2001, pp. 1223-1236
Authors:
Webb, JK
Murphy, MT
Flambaum, VV
Dzuba, VA
Barrow, JD
Churchill, CW
Prochaska, JX
Wolfe, AM
Citation: Jk. Webb et al., Further evidence for cosmological evolution of the fine structure constant- art. no. 091301, PHYS REV L, 8709(9), 2001, pp. 1301
Authors:
Bond, NA
Churchill, CW
Charlton, JC
Vogt, SS
Citation: Na. Bond et al., High-redshift superwinds as the source of the strongest MgII absorbers: A feasibility analysis, ASTROPHYS J, 562(2), 2001, pp. 641-648
Citation: Cw. Churchill, Mg II absorber number density at z similar or equal to 0.05: Implications for Omega(DLA) evolution, ASTROPHYS J, 560(1), 2001, pp. 92-100
Authors:
Bouche, N
Lowenthal, JD
Charlton, JC
Bershady, MA
Churchill, CW
Steidel, CC
Citation: N. Bouche et al., H alpha imaging with Hubble Space Telescope-NICMOS of an elusive damped Lyalpha cloud at z=0.6, ASTROPHYS J, 550(2), 2001, pp. 585-592
Authors:
Ganguly, R
Bond, NA
Charlton, JC
Eracleous, M
Brandt, WN
Churchill, CW
Citation: R. Ganguly et al., On the origin of intrinsic narrow absorption lines in z less than or similar to 1 QSOs, ASTROPHYS J, 549(1), 2001, pp. 133-154
Authors:
Churchill, CW
Mellon, RR
Charlton, JC
Jannuzi, BT
Kirhakos, S
Steidel, CC
Schneider, DP
Citation: Cw. Churchill et al., Low- and high-ionization absorption properties of MgII absorption-selectedgalaxies at intermediate redshifts. I. General properties, ASTROPH J S, 130(1), 2000, pp. 91-119
Authors:
Charlton, JC
Mellon, RR
Rigby, JR
Churchill, CW
Citation: Jc. Charlton et al., Anticipating high-resolution STIS spectra of four multiphase MgII absorbers: A test of photoionization models, ASTROPHYS J, 545(2), 2000, pp. 635-656
Authors:
Churchill, CW
Mellon, RR
Charlton, JC
Jannuzi, BT
Kirhakos, S
Steidel, CC
Schneider, DP
Citation: Cw. Churchill et al., Low- and high-ionization absorption properties of MgII absorption-selectedgalaxies at intermediate redshifts. II. Taxonomy, kinematics, and galaxies, ASTROPHYS J, 543(2), 2000, pp. 577-598
Authors:
Churchill, CW
Mellon, RR
Charlton, JC
Jannuzi, BT
Kirhakos, S
Steidel, CC
Schneider, DP
Citation: Cw. Churchill et al., The C IV absorption-Mg II kinematics connection in < z > similar to 0.7 galaxies, ASTROPHYS J, 519(1), 1999, pp. L43-L46
Citation: Cw. Churchill et Jc. Charlton, The multiple phases of interstellar and halo gas in a possible group of galaxies at z similar to 1, ASTRONOM J, 118(1), 1999, pp. 59-75
Authors:
Ganguly, R
Eracleous, M
Charlton, JC
Churchill, CW
Citation: R. Ganguly et al., Intrinsic narrow absorption lines in keck hires spectra of a sample of sixquasars, ASTRONOM J, 117(6), 1999, pp. 2594-2607