The Connection between a Lyman Limit System, a very strong O VI Absorber, and Galaxies at z∼ 0.203
N Lehner, JX Prochaska, HA Kobulnicky… - The Astrophysical …, 2009 - iopscience.iop.org
With a column density log N (O vi)= 14.95±0.05, the O vi absorber at z abs≃ 0.2028
observed toward the quasi-stellar object PKS 0312–77 (z em= 0.223) is the strongest yet …
observed toward the quasi-stellar object PKS 0312–77 (z em= 0.223) is the strongest yet …
[PDF][PDF] THE CONNECTION BETWEEN A LYMAN LIMIT SYSTEM, A VERY STRONG O VI ABSORBER, AND GALAXIES AT Z∼ 0.2031
N Lehner, JX Prochaska, HA Kobulnicky… - arXiv preprint arXiv …, 2008 - researchgate.net
With a column density log N (O VI)= 14.95±0.05, the O VI absorber at zabs≃ 0.2028
observed toward the QSO PKS 0312–77 (zem= 0.223) is the strongest yet detected at z< 0.5 …
observed toward the QSO PKS 0312–77 (zem= 0.223) is the strongest yet detected at z< 0.5 …
The Connection Between a Lyman Limit System, a Very Strong O VI Absorber, and Galaxies at z~ 0.203
N Lehner, JX Prochaska… - The Astrophysical …, 2009 - ui.adsabs.harvard.edu
With a column density log N (O VI)= 14.95±0.05, the O VI absorber at z abs sime 0.2028
observed toward the quasi-stellar object PKS 0312-77 (z em= 0.223) is the strongest yet …
observed toward the quasi-stellar object PKS 0312-77 (z em= 0.223) is the strongest yet …
The Connection between a Lyman Limit System, a very strong OVI Absorber, and Galaxies at z~ 0.203
N Lehner, JX Prochaska, HA Kobulnicky, KL Cooksey… - Astrophys. J., 2009 - inspirehep.net
With a column density log N (OVI)= 14.95+/-0.05, the OVI absorber at z_abs~ 0.2028
observed toward the QSO PKS0312-77 (z_em= 0.223) is the strongest yet detected at z< …
observed toward the QSO PKS0312-77 (z_em= 0.223) is the strongest yet detected at z< …
THE CONNECTION BETWEEN A LYMAN LIMIT SYSTEM, A VERY STRONG O VI ABSORBER, AND GALAXIES AT z∼ 0.203
N Lehner, JC Howk, JX Prochaska, KL Cooksey… - Astrophysical …, 2009 - inis.iaea.org
[en] With a column density log N (O VI)= 14.95±0.05, the O VI absorber at z abs≅ 0.2028
observed toward the quasi-stellar object PKS 0312-77 (z em= 0.223) is the strongest yet …
observed toward the quasi-stellar object PKS 0312-77 (z em= 0.223) is the strongest yet …
[引用][C] THE CONNECTION BETWEEN A LYMAN LIMIT SYSTEM, A VERY STRONG O VI ABSORBER, AND GALAXIES AT z∼ 0.203
N LEHNER, JX PROCHASKA… - The Astrophysical …, 2009 - pascal-francis.inist.fr
THE CONNECTION BETWEEN A LYMAN LIMIT SYSTEM, A VERY STRONG O VI
ABSORBER, AND GALAXIES AT z ∼ 0.203 CNRS Inist Pascal-Francis CNRS Pascal and …
ABSORBER, AND GALAXIES AT z ∼ 0.203 CNRS Inist Pascal-Francis CNRS Pascal and …
[PDF][PDF] THE CONNECTION BETWEEN A LYMAN LIMIT SYSTEM, A VERY STRONG OVI ABSORBER, AND GALAXIES AT z∼ 0.203
N LEHNER, JX PROCHASkA, HA KOBULNICkY… - THE ASTROPHYSICAL …, 2009 - Citeseer
With a column density log N (O VI)= 14.95±0.05, the O VI absorber at zabs≃ 0.2028
observed toward the quasi-stellar object PKS 0312–77 (zem= 0.223) is the strongest yet …
observed toward the quasi-stellar object PKS 0312–77 (zem= 0.223) is the strongest yet …
The Connection between a Lyman Limit System, a very strong OVI Absorber, and Galaxies at z~ 0.203
N Lehner, JX Prochaska, HA Kobulnicky… - arXiv preprint arXiv …, 2008 - arxiv.org
With a column density log N (OVI)= 14.95+/-0.05, the OVI absorber at z_abs~ 0.2028
observed toward the QSO PKS0312-77 (z_em= 0.223) is the strongest yet detected at z< …
observed toward the QSO PKS0312-77 (z_em= 0.223) is the strongest yet detected at z< …
[PDF][PDF] THE CONNECTION BETWEEN A LYMAN LIMIT SYSTEM, A VERY STRONG OVI ABSORBER, AND GALAXIES AT z∼ 0.203
N LEHNER, JX PROCHASkA… - THE …, 2009 - scholar.archive.org
With a column density log N (O VI)= 14.95±0.05, the O VI absorber at zabs≃ 0.2028
observed toward the quasi-stellar object PKS 0312–77 (zem= 0.223) is the strongest yet …
observed toward the quasi-stellar object PKS 0312–77 (zem= 0.223) is the strongest yet …