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Galactic Scale Feedback Observed in the 3C 298 Quasar Host Galaxy

, , , , , and . (2017)cite arxiv:1709.03510Comment: 23 pages, 11 figures, 4 tables, submitted to the Astrophysical Journal.

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Accretion Does Not Drive the Turbulence in Galactic Disks, , and . (2013)cite arxiv:1301.4500Comment: 7 pages, 3 figures, submitted to MNRAS.Dense Molecular Gas: A Sensitive Probe of Stellar Feedback Models, , , and . (2012)cite arxiv:1209.0459Comment: 6 pages, 2 figures, submitted to MNRAS.Forged in FIRE: cusps, cores, and baryons in low-mass dwarf galaxies, , , , , , , and . (2015)cite arxiv:1502.02036Comment: 16 pages, 12 figures, submitted to MNRAS. Comments welcome.What FIREs Up Star Formation: the Emergence of the Kennicutt-Schmidt Law from Feedback, , , , , , , , and . (2017)cite arxiv:1701.01788Comment: 15 pages, 10 figures, submitted to MNRAS.Binary Stars Can Provide the "Missing Photons" Needed for Reionization, , , , , , and . (2016)cite arxiv:1601.07559Comment: 6 pages, 3 figures, submitted to MNRAS Letter.Kaleidoscape: A 3D Environment for Querying ODMG Compliant Databases., , and . VDB, volume 126 of IFIP Conference Proceedings, page 85-101. Chapman & Hall, (1998)When Feedback Fails: The Scaling and Saturation of Star Formation Efficiency, , , , , and . (2016)cite arxiv:1612.05635Comment: Submitted to MNRAS; 16 pages, 6 figures.Scattered Emission from z~1 Galactic Outflows, , , , , and . (2013)cite arxiv:1304.6405Comment: Manuscript accepted for publication in the Astrophysical Journal. The 22 pages include 2 tables, 10 figures, and an Appendix.The Structure of the Interstellar Medium of Star Forming Galaxies, , and . (2011)cite arxiv:1110.4636 Comment: 34 pages, 23 figures, submitted to MNRAS. Movies of the simulations are available at https://www.cfa.harvard.edu/~phopkins/Site/Movies_sbw.html.The Difficulty Getting High Escape Fractions of Ionizing Photons from High-redshift Galaxies: a View from the FIRE Cosmological Simulations, , , , , , and . (2015)cite arxiv:1503.07880Comment: 16 pages, 14 figures, submitted to MNRAS; comments welcome.