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Cited by 95 publications
(124 citation statements)
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“…The first 3-D calculations of the shock-cloud interaction showed a richer structure of the hydrodynamic instabilities (Stone & Norman 1992;Xu & Stone 1995). The 3-D calculations do not invalidate any of the conclusions drawn from the 2-D calculations; however, they showed that the cloud breaks in all directions and that the turbulent mixing of the cloud and the interstellar medium is complete, with the formation of macroscopic vortex filaments.…”
Section: Introductionmentioning
confidence: 90%
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“…The first 3-D calculations of the shock-cloud interaction showed a richer structure of the hydrodynamic instabilities (Stone & Norman 1992;Xu & Stone 1995). The 3-D calculations do not invalidate any of the conclusions drawn from the 2-D calculations; however, they showed that the cloud breaks in all directions and that the turbulent mixing of the cloud and the interstellar medium is complete, with the formation of macroscopic vortex filaments.…”
Section: Introductionmentioning
confidence: 90%
“…KMC94 showed that the most disruptive wavelengths are those corresponding to k λ r cl ∼ 1. If not suppressed, these instabilities are responsible for cloud break-up on time-scales comparable with τ cc , eventually leading to efficient mixing of the cloud material with its surrounding and to the final cloud destruction (see also Xu & Stone 1995;Poludnenko et al 2002).…”
Section: Time-scalesmentioning
confidence: 99%
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“…M A is the Alfvénic Mach number, M slow/fast are the slow/fast magnetosonic Mach numbers. t cc is the cloud-crushing time-scale of Klein et al (1994), while t cs is the cloud-crushing time-scale for a spherical cloud of equivalent mass introduced by Xu & Stone (1995). Key filament time-scales are additionally noted.…”
Section: Filament Morphologymentioning
confidence: 99%
“…Such studies can be used to under-⋆ Corresponding author: e-mail: sjk@astro.ugto.mx stand the relation between the outflow and the ionisation of the gas. In fact, several numerical studies have been attempted to study the interaction of the jets with clouds in the ambient medium (Choi, Wiita, & Ryu 2007;Fragile et al 2004;Higgins, O'Brien, & Dunlop 1999;Wang, Wiita, & Hooda 2000;Xu & Stone 1995). All these studies focused on the evolution of the individual clouds and the effect of the clouds on the dynamics and morphology of the radio source.…”
Section: Introductionmentioning
confidence: 99%