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The Relationship Between Molecular Gas, HI, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds

, , , , , , , , , , , , , , , , and . (2015)cite arxiv:1510.08084Comment: 24 pages, 14 figures, submitted for publication in ApJ.

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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 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.The importance of Wolf-Rayet ionization and feedback on super star cluster evolution, , , and . (2015)cite arxiv:1508.00572Comment: To appear in the conference proceedings of the June 2015 Potsdam Wolf-Rayet workshop, edited by W.-R. Hamann, A. Sander, and H. Todt. 3 pages, 3 figures.Molecular hydrogen emission in the interstellar medium of the Large Magellanic Cloud, , , , , , , , , and 13 other author(s). (2014)cite arxiv:1407.7658Comment: Submitted to MNRAS.Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission, , , , , , , , , and 26 other author(s). (2014)cite arxiv:1406.6066Comment: 20 pages, 9 figures, accepted for publication in the ApJ.New Insights into the Physical Conditions and Internal Structure of a Candidate Proto-Globular Cluster, , , , , , , and . (2019)cite arxiv:1903.08669Comment: 18 pages, 14 figures, Accepted to ApJ 2019 March 4.