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Carbon Monoxide Clouds at Low-Metallicity in the WLM Galaxy

, , , , , и . (2013)cite arxiv:1310.4322Comment: 9 pages, 3 tables, 1 figure.

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Andreas Schruba

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Carbon Monoxide Clouds at Low-Metallicity in the WLM Galaxy, , , , , и . (2013)cite arxiv:1310.4322Comment: 9 pages, 3 tables, 1 figure.Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way, , , , , , , , и . (2017)cite arxiv:1701.02748Comment: Accepted for publication in The Astrophysical Journal; 22 pages, 10 figures, 7 tables.A model for the onset of self-gravitation and star formation in molecular gas governed by galactic forces: II. the bottleneck to collapse set by cloud-environment decoupling, , , , , , , , , и 5 other автор(ы). (2020)cite arxiv:2001.07459Comment: Accepted for publication in ApJ, 32 pages, 11 figures.The chemical evolution of local star forming galaxies: Radial profiles of ISM metallicity, gas mass, and stellar mass and constraints on galactic accretion and winds, , , , , , и . (2015)cite arxiv:1503.01503Comment: 19 pages, 17 figure, accepted to MNRAS.High-resolution mass models of dwarf galaxies from LITTLE THINGS, , , , , , , , , и 6 other автор(ы). (2015)cite arxiv:1502.01281Comment: 100 pages, 85 figures, Accepted for publication on AJ.A Molecular Star Formation Law in the Atomic Gas Dominated Regime in Nearby Galaxies, , , , , , , , , и 4 other автор(ы). (2011)cite arxiv:1105.4605Comment: Accepted for publication in the Astronomical Journal, 28 pages, 25 figures.Clumping and the Interpretation of kpc-Scale Maps of the Interstellar Medium: Smooth HI and Clumpy, Variable H2 Surface Density, , , , , , , , и . (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, , , , , , и . (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.