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The Role of Stellar Feedback in the Dynamics of HII Regions

, , , , , and . (2013)cite arxiv:1309.5421Comment: 18 pages, 8 figures; submitted to ApJ.

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Formation of Molecular Clouds and Global Conditions for Star Formation, , , , , , , , and . (2013)cite arxiv:1312.3223Comment: 25 pages, 7 figures, Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. Klessen, C. Dullemond, Th. Henning.ALFALFA Discovery of the Nearby Gas-rich Dwarf Galaxy Leo P. V. Neutral Gas Dynamics and Kinematics, , , , , , , , , and 4 other author(s). (2014)cite arxiv:1404.5298Comment: 38 pages, 11 figures, Accepted for publication in the Astronomical Journal.The State of the Gas and the Relation Between Gas and Star Formation at Low Metallicity: the Small Magellanic Cloud, , , , , , , , , and 8 other author(s). (2011)cite arxiv:1107.1717Comment: Accepted for publication in the Astrophysical Journal. 21 pages and 11 figures in apjemulate style.Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview, , , , , , , , , and 50 other author(s). (2011)cite arxiv:1107.4313Comment: 16 pages, 11 figures, AJ, in press.The Role of Stellar Feedback in the Dynamics of HII Regions, , , , , and . (2013)cite arxiv:1309.5421Comment: 18 pages, 8 figures; submitted to ApJ.The Relationship Between Molecular Gas, HI, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1510.08084Comment: 24 pages, 14 figures, submitted for publication in ApJ.The Parsec-Scale Relationship Between I_CO and A_V in Local Molecular Clouds, , , , , , and . (2017)cite arxiv:1710.08435Comment: Accepted for publication in MNRAS, 16 pages, 9 figures in main text, manuscript also includes a 24 page atlas showing each cloud. Full resolution available here: http://www.astronomy.ohio-state.edu/~leroy.42/MW_Planck_ICO_AV.pdf.Formation of Molecular Clouds and Global Conditions for Star Formation, , , , , , , , and . (Dec 11, 2013)The Multi-Phase Cold Fountain in M82 Revealed by a Wide, Sensitive Map of the Molecular ISM, , , , , , , , , and . (2015)cite arxiv:1509.02932Comment: 36 pages including 25 figures and 4 appendices. Accepted for publication in the Astrophysical Journal. For a high resolution version please visit http://www.astronomy.ohio-state.edu/~leroy.42/ms_m82.pdf.The CO-to-H2 Conversion Factor, , and . (2013)cite arxiv:1301.3498Comment: To appear in ARAA, Annual Reviews of Astronomy and Astrophysics, ARAA issue 51. This instance is compiled in ApJ format, 35 pages, 12 figures (most in color).