Zobrazeno 1 - 10
of 81
pro vyhledávání: '"S. A. E. G. Falle"'
Using the adaptive mesh refinement code mg, we perform hydrodynamic simulations of the interaction of a shock with a molecular cloud evolving due to thermal instability (TI) and gravity. To explore the relative importance of these processes, three ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88dd5e1987d3f9011cdc2c282fd89139
https://eprints.whiterose.ac.uk/169465/1/2012.04546v1.pdf
https://eprints.whiterose.ac.uk/169465/1/2012.04546v1.pdf
The MHD version of the adaptive mesh refinement (AMR) code, MG, has been employed to study the interaction of thermal instability, magnetic fields and gravity through 3D simulations of the formation of collapsing cold clumps on the scale of a few par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a47c535ba8914a73bebe1c611cbbdbd
https://eprints.whiterose.ac.uk/167579/1/ms2020_magcollapse_R3.pdf
https://eprints.whiterose.ac.uk/167579/1/ms2020_magcollapse_R3.pdf
Field's linear analysis of thermal instability is repeated using methods related to Whitham's theory of wave hierarchies, which brings out the physically relevant parameters in a much clearer way than in the original analysis. It is also used for the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4410422f18d5bcc3cef963080d1b8f31
This paper describes 3D simulations of the formation of collapsing cold clumps via thermal instability inside a larger cloud complex. The initial condition was a diffuse atomic, stationary, thermally unstable, 200pc diameter spherical cloud in pressu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6436ba98ff11ca8458a90ad2b24d7ca7
http://arxiv.org/abs/1812.09051
http://arxiv.org/abs/1812.09051
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 465:2757-2783
We have used the AMR hydrodynamic code, MG, to perform 3D magnetohydrodynamic simulations with self-gravity of stellar feedback in a sheet-like molecular cloud formed through the action of the thermal instability. We simulate the interaction of the m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e0b80070fbbc063a3625c2f98a554105
https://doi.org/10.1093/mnras/stw2990
https://doi.org/10.1093/mnras/stw2990
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 465:260-268
We describe the results of 3D simulations of the interaction of hydrodynamic shocks with Bonnor-Ebert spheres performed with an Adaptive Mesh Refinement code. The calculations are isothermal and the clouds are embedded in a medium in which the sound
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b79ecee64cc64943f1b625f9c24c9699
https://doi.org/10.1093/mnras/stw2795
https://doi.org/10.1093/mnras/stw2795
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 459:1803-1818
We have used the AMR hydrodynamic code, MG, to perform idealised 3D MHD simulations of the formation of clumpy and filamentary structure in a thermally unstable medium without turbulence. A stationary thermally unstable spherical diffuse atomic cloud
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a8f76a90c22b6c7639c90b8d70e07be1
https://doi.org/10.1093/mnras/stw581
https://doi.org/10.1093/mnras/stw581
Autor:
Robert M. Woolley, Christopher J. Wareing, S. A. E. G. Falle, Michael Fairweather, Jeff Peakall
Publikováno v:
Procedia Engineering. 102:1621-1629
Under-expanded particle-laden flows resulting in velocities greater than the local speed of sound are a feature of a wide number of applications in aviatic, astronautical, and process engineering scenarios including those relating to the accidental r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e694330ad94f175a209f5129e8158515
https://doi.org/10.1016/j.proeng.2015.01.298
https://doi.org/10.1016/j.proeng.2015.01.298
We have used the AMR hydrodynamic code, MG, to perform 3D hydrodynamic simulations with self-gravity of stellar feedback in a spherical clumpy molecular cloud formed through the action of thermal instability. We simulate the interaction of the mechan
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4652460ae50422b9da2dfd6a2fef5c49
Autor:
Idar E. Storvik, Christophe Proust, Jérôme Hebrard, Michael Fairweather, S E Gant, Christopher J. Wareing, Dimitrios M. Tsangaris, Didier Jamois, Trygve Skjold, Georgios C. Boulougouris, Nikolaos I. Diamantonis, Haroun Mahgerefteh, Vagesh D. Narasimhamurthy, S. A. E. G. Falle, Sergey Martynov, Solomon Brown, Ioannis G. Economou, Robert M. Woolley
Publikováno v:
International Journal of Greenhouse Gas Control. 27:221-238
The deployment of a complete carbon capture and storage chain requires a focus upon the hazards posed by the operation of pipelines transporting carbon dioxide (CO2) at high pressure in a dense-phase (supercritical or liquid state). The consequences
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5a489512391d69508d7021eb17f8cf4
https://doi.org/10.1016/j.ijggc.2014.06.001
https://doi.org/10.1016/j.ijggc.2014.06.001