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Exploring the Properties of Warm and Cold Atomic Hydrogen in the Taurus and Gemini Regions
Hiep Nguyen, J. R. Dawson, Min-Young Lee, Claire E. Murray, Snežana Stanimirović, Carl Heiles, M.-A. Miville-Deschênes and Anita Hafner The Astrophysical Journal 880(2) 141 (2019) https://doi.org/10.3847/1538-4357/ab2b9f
On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions
P R Joshi, S Walch, D Seifried, et al. Monthly Notices of the Royal Astronomical Society 484(2) 1735 (2019) https://doi.org/10.1093/mnras/stz052
Sheets, filaments, and clumps – high-resolution simulations of how the thermal instability can form molecular clouds
C J Wareing, S A E G Falle and J M Pittard Monthly Notices of the Royal Astronomical Society 485(4) 4686 (2019) https://doi.org/10.1093/mnras/stz768
Triggering the formation of the supergiant H ii region NGC 604 in M 33
Kengo Tachihara, Pierre Gratier, Hidetoshi Sano, Kisetsu Tsuge, Rie E Miura, Kazuyuki Muraoka and Yasuo Fukui Publications of the Astronomical Society of Japan 70(SP2) (2018) https://doi.org/10.1093/pasj/psy020
Star formation induced by cloud–cloud collisions and galactic giant molecular cloud evolution
Masato I N Kobayashi, Hiroshi Kobayashi, Shu-ichiro Inutsuka and Yasuo Fukui Publications of the Astronomical Society of Japan 70(SP2) (2018) https://doi.org/10.1093/pasj/psy018
Atomic and Ionized Microstructures in the Diffuse Interstellar Medium
Velocity-resolved [
] Emission from Cold Diffuse Clouds in the Interstellar Medium
Paul F. Goldsmith, Jorge L. Pineda, David A. Neufeld, Mark G. Wolfire, Christophe Risacher and Robert Simon The Astrophysical Journal 856(2) 96 (2018) https://doi.org/10.3847/1538-4357/aab34e
Evolutionary Description of Giant Molecular Cloud Mass Functions on Galactic Disks
Recovering Interstellar Gas Properties with Hi Spectral Lines: A Comparison between Synthetic Spectra and 21-SPONGE
Claire E. Murray, Snežana Stanimirović, Chang-Goo Kim, Eve C. Ostriker, Robert R. Lindner, Carl Heiles, John M. Dickey and Brian Babler The Astrophysical Journal 837(1) 55 (2017) https://doi.org/10.3847/1538-4357/aa5d12
Structure formation in a colliding flow: The Herschel view of the Draco nebula
FORMATION OF H i CLOUDS IN SHOCK-COMPRESSED INTERSTELLAR MEDIUM: PHYSICAL ORIGIN OF ANGULAR CORRELATION BETWEEN FILAMENTARY STRUCTURE AND MAGNETIC FIELD
Molecular cloud formation as seen in synthetic H i and molecular gas observations
Jonathan S. Heiner, Enrique Vázquez-Semadeni and Javier Ballesteros-Paredes Monthly Notices of the Royal Astronomical Society 452(2) 1353 (2015) https://doi.org/10.1093/mnras/stv1153
The onset of large-scale turbulence in the interstellar medium of spiral galaxies
D. Falceta-Gonçalves, I. Bonnell, G. Kowal, J. R. D. Lépine and C. A. S. Braga Monthly Notices of the Royal Astronomical Society 446(1) 973 (2015) https://doi.org/10.1093/mnras/stu2127
nbody6++gpu: ready for the gravitational million-body problem
Long Wang, Rainer Spurzem, Sverre Aarseth, et al. Monthly Notices of the Royal Astronomical Society 450(4) 4070 (2015) https://doi.org/10.1093/mnras/stv817
Star formation in the first galaxies – II. Clustered star formation and the influence of metal line cooling
Chalence Safranek-Shrader, Miloš Milosavljević and Volker Bromm Monthly Notices of the Royal Astronomical Society 438(2) 1669 (2014) https://doi.org/10.1093/mnras/stt2307
The structure of the thermally bistable and turbulent atomic gas in the local interstellar medium
The structure of H i in galactic discs: simulations versus observations
David M. Acreman, Clare L. Dobbs, Christopher M. Brunt and Kevin A. Douglas Monthly Notices of the Royal Astronomical Society 422(1) 241 (2012) https://doi.org/10.1111/j.1365-2966.2012.20599.x
FORMATION OF TURBULENT AND MAGNETIZED MOLECULAR CLOUDS VIA ACCRETION FLOWS OF H I CLOUDS
Cooling, Gravity, and Geometry: Flow‐driven Massive Core Formation
Fabian Heitsch, Lee W. Hartmann, Adrianne D. Slyz, Julien E. G. Devriendt and Andreas Burkert The Astrophysical Journal 674(1) 316 (2008) https://doi.org/10.1086/523697
The ISM in spiral galaxies: can cooling in spiral shocks produce molecular clouds?
