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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 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.Carbon Monoxide Clouds at Low-Metallicity in the WLM Galaxy, , , , , and . (2013)cite arxiv:1310.4322Comment: 9 pages, 3 tables, 1 figure.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.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.Jittering Reduction in Marker-Based Augmented Reality Systems., , , , and . ICCSA (1), volume 3980 of Lecture Notes in Computer Science, page 510-517. Springer, (2006)