The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.
Thermal condensation in a turbulent atomic hydrogen flow
Open accessAbstract
We present a numerical and analytical study of the thermal fragmentation of a turbulent flow of interstellar hydrogen. We first present the different dynamical processes and the large range of spatial (and temporal) scales that need to be adequately represented in numerical simulations. Next, we present bidimensional simulations of turbulent converging flows which induce the dynamical condensation of the warm neutral phase into the cold phase. We then analyse the cold structures and the fraction of unstable gas in each simulation, paying particular attention to the influence of the degree of turbulence. When the flow is very turbulent a large fraction of the gas remains in the thermally unstable domain. This unstable gas forms a filamentary network. We show that the fraction of thermally unstable gas is strongly correlated with the level of turbulence of the flow. We then develop a semi-analytical model to explain the origin of this unstable gas. This simple model is able to quantitatively reproduce the fraction of unstable gas observed in the simulations and its correlation with turbulence. Finally, we stress the fact that even when the flow is very turbulent and in spite of the fact that a large fraction of the gas is maintained dynamically in the thermally unstable domain, the classical picture of a 2-phase medium with stiff thermal fronts and local pressure equilibrium turns out to be still relevant in the vicinity of the cold structures.
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BackgroundField, G. B. (1965) · The Astrophysical Journal · doi:10.1086/148317 · Cited by 1,419
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Draine, B. T. (1978) · The Astrophysical Journal Supplement Series · doi:10.1086/190513 · Cited by 1,342
Neutral Atomic Phases of the Interstellar Medium in the Galaxy
Wolfire, M. G., McKee, C. F., Hollenbach, D., & Tielens, A. G. G. M. (2003) · The Astrophysical Journal · doi:10.1086/368016 · Cited by 1,125
The neutral atomic phases of the interstellar medium
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Cosmic-Ray Heating of the Interstellar Gas
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Infrared cirrus - New components of the extended infrared emission
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Science with ASKAP: The Australian square-kilometre-array pathfinder
Johnston, S., Taylor, R., Bailes, M., Bartel, N., Baugh, C., Bietenholz, M., Blake, C., Braun, R., Brown, J., Chatterjee, S., et al. (2008) · Experimental Astronomy · doi:10.1007/s10686-008-9124-7 · Cited by 409
Global hierarchical collapse in molecular clouds. Towards a comprehensive scenario
Vázquez-Semadeni, E., Palau, A., Ballesteros-Paredes, J., Gómez, G. C., & Zamora-Avilés, M. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2736 · Cited by 361
Redfield, S., & Linsky, J. L. (2008) · The Astrophysical Journal · doi:10.1086/524002 · Cited by 358
Accretion-driven turbulence as universal process: galaxies, molecular clouds, and protostellar disks
Klessen, R. S., & Hennebelle, P. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913780 · Cited by 301
Self-citationScience with ASKAP - the Australian Square Kilometre Array Pathfinder
Johnston, S., Taylor, R., Bailes, M., Bartel, N., Baugh, C. M., Bietenholz, M. F., Blake, C., Braun, R. L., Brown, J. C., Chatterjee, S., et al. (2008) · arXiv (Cornell University) · doi:10.48550/arxiv.0810.5187 · Cited by 254
Metadata
- Authors
- Audit, E., & Hennebelle, P.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2005-03-14
- Volume
- 433
- Issue
- 1
- Pages
- 1-13
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2951458773
- Cited by
- 353
- References
- 23
- FWCI
- 13.27
- Type
- journal article
- Language
- en
- Open access
- bronze
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