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Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies

, , , , , , , , and . (2015)cite arxiv:1510.06410Comment: 13 pages, 6 figures. Submitted to MNRAS.

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Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies, , , , , , , , and . (2015)cite arxiv:1510.06410Comment: 13 pages, 6 figures. Submitted to MNRAS.A Stellar Feedback Origin for Neutral Hydrogen in High-Redshift Quasar-Mass Halos, , , , , and . (2016)cite arxiv:1601.07188Comment: 6 pages, including 3 figures. Submitted.Predictions for the spatial distribution of the dust continuum emission in 1<z<5 star-forming galaxies, , , , , , , , and . (2019)cite arxiv:1905.13234Comment: 12 pages, 8 figures; accepted for publication in MNRAS.The Impact of Baryonic Physics on the Structure of Dark Matter Halos: the View from the FIRE Cosmological Simulations, , , , , , and . (2015)cite arxiv:1507.02282Comment: 23 pages, 14 figures, submitted to MNRAS.Photon-Mediated Sequential Resonant Tunneling in Intense Terahertz Electric Fields, , , , , , , and . Phys.~Rev.~Lett., (1993)Low-Redshift Lyman Limit Systems as Diagnostics of Cosmological Inflows and Outflows, , , , , , , , and . (2016)cite arxiv:1608.05712Comment: 13 pages, 12 figures. Submitted.Turbulent Disks are Never Stable: Fragmentation and Turbulence-Promoted Planet Formation, and . ArXiv e-prints, (January 2013)Temperature and Intensity Dependence of Intersubband Relaxation Rates from Photovoltage and Absorption, , , , , , , and . Phys.~Rev.~Lett., 74 (4): 2682--2685 (1995)Galaxy disks do not need to survive in the L-CDM paradigm: the galaxy merger rate out to z\sim1.5 from morpho-kinematic data, , , , , , , and . (2012)cite arxiv:1206.0008Comment: 19 pages, 7 figures, 2 tables. Accepted for publication in ApJ.