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A Molecular Star Formation Law in the Atomic Gas Dominated Regime in Nearby Galaxies

, , , , , , , , , , , , , and . (2011)cite arxiv:1105.4605Comment: Accepted for publication in the Astronomical Journal, 28 pages, 25 figures.

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The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group, , , , , , , , , and 1 other author(s). (2011)cite arxiv:1102.4618 Comment: Accepted for publication in the Astrophysical Journal, 15 pages, 7 figures.A Molecular Star Formation Law in the Atomic Gas Dominated Regime in Nearby Galaxies, , , , , , , , , and 4 other author(s). (2011)cite arxiv:1105.4605Comment: Accepted for publication in the Astronomical Journal, 28 pages, 25 figures.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.Clumping and the Interpretation of kpc-Scale Maps of the Interstellar Medium: Smooth HI and Clumpy, Variable H2 Surface Density, , , , , , , , and . (2013)cite arxiv:1304.1586Comment: 6 pages, 2 figures, accepted for publication in ApJ Letters.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.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.Andromeda's Dust, , , , , , , , , and 3 other author(s). (2013)cite arxiv:1306.2304Comment: 36 pages, 14 figures. Submitted to ApJ.The heating of dust by old stellar populations in the Bulge of M31, , , , , , , , , and 2 other author(s). (2012)cite arxiv:1206.2925Comment: 11 pages. Accepted for publication in MNRAS.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.PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula, , , , , , , , , and 132 other author(s). (2023)cite arxiv:2308.16732.