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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 . (2011)cite arxiv:1107.1717Comment: Accepted for publication in the Astrophysical Journal. 21 pages and 11 figures in apjemulate style.

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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 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.Far-ultraviolet Dust Extinction and Molecular Hydrogen in the Diffuse Milky Way Interstellar Medium, , , , and . (2022)cite arxiv:2210.04972Comment: 24 pages, 9 figures, accepted for publication in ApJ.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.Dust-to-Gas Ratio in the Extremely Metal Poor Galaxy I ZW 18, , , , , , , , , and . (2012)cite arxiv:1204.4745Comment: Accepted for publication in ApJ: 8 pages, 4 figures, 1 table.PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula, , , , , , , , , and 132 other author(s). (2023)cite arxiv:2308.16732.PDRs4All III: JWST's NIR spectroscopic view of the Orion Bar, , , , , , , , , and 128 other author(s). (2023)cite arxiv:2310.08720Comment: 52 pages, 30 figures, submitted to A&A.