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An Origin for Multi-Phase Gas in Galactic Winds and Halos

, , , and . (2015)cite arxiv:1507.04362Comment: 15 pages, 5 figures, submitted. Comments welcome.

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The Close Binary Fraction as a Function of Stellar Parameters in APOGEE: A Strong Anti-Correlation With $\alpha$ Abundances, , , , , , , , , and 11 other author(s). (2020)cite arxiv:2007.09059Comment: 15 pages, 10 figures, plus appendices; submitted to MNRAS.Highly-mass-loaded hot galactic winds are unstable to cool filament formation, , , and . (2023)cite arxiv:2307.11930Comment: 12 pages, 15 figures, submitted to MNRAS (21 July 2023).An Origin for Multi-Phase Gas in Galactic Winds and Halos, , , and . (2015)cite arxiv:1507.04362Comment: 15 pages, 5 figures, submitted. Comments welcome.A Brief Review of Galactic Winds, and . (2017)cite arxiv:1701.09062Comment: Book chapter for 'Handbook of Supernovae,' edited by Alsabti and Murdin, Springer. 24 pages, 3 figures.The Impact of Star Formation Feedback on the Circumgalactic Medium, , , and . (2016)cite arxiv:1606.06734Comment: submitted to MNRAS, 18 pages, 18 figures, comments welcome.Entrainment in Trouble: Cool Cloud Acceleration and Destruction in Hot Supernova-Driven Galactic Winds, , , and . (Jul 7, 2015)A Unicorn in Monoceros: the $3M_ødot$ dark companion to the bright, nearby red giant V723 Mon is a non-interacting, mass-gap black hole candidate, , , , , , , , , and 11 other author(s). (2021)cite arxiv:2101.02212Comment: 25 pages, 14 figures. Will be submitted to MNRAS. Comments welcome.Short GMC lifetimes: an observational estimate with the PdBI Arcsecond Whirlpool Survey (PAWS), , , , , , , , , and 3 other author(s). (2015)cite arxiv:1504.04528Comment: 16 pages, 8 figures, accepted for publication in ApJ.Numerical Simulations of Radiatively-Driven Dusty Winds, and . (2013)cite arxiv:1302.4440Comment: 16 pages, 14 figures, submitted to MNRAS.Sub-Eddington Star-Forming Regions are Super-Eddington: Momentum Driven Outflows from Supersonic Turbulence, and . (2014)cite arxiv:1411.1769Comment: 9 pages, 5 figures. Submitted. Comments welcome.