Hydrodynamic Modeling of the Interaction of Winds within a Collapsing Turbulent Gas Cloud

<div>For the last snapshot available for each simulation, we show the accretion centers detected with the density <svg height="11.6478pt" id="M262" style="vertical-align:-3.40336pt" version="1.1" viewbox="-0.0498162 -8.24444 56.0432 11.6478" width="56.0432pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.013,0,0,-0.013,0,0)"><path d="M525 275C525 381 464 451 380 451C338 451 289 439 241 405C158 347 127 277 106 152C51 -168 37 -216 24 -242L28 -257C42 -256 92 -247 117 -222C126 -213 134 -193 150 -69L166 32C184 10 211 -12 245 -12C276 -12 332 8 384 46C458 100 525 176 525 275ZM436 260C436 131 366 41 267 41C246 41 208 51 175 82C181 125 187 162 195 200C220 322 257 400 328 400C398 400 436 338 436 260Z" id="g50-239"></path><glyph.data ascent="3443" descent="-2856" horiz-adv-x="549" vert-adv-y="549"></glyph.data></g><g transform="matrix(.0091,0,0,-0.0091,6.292,3.001)"><path d="M357 391C357 416 325 451 270 451C241 451 179 431 146 400C109 365 97 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Advances in Astronomy

fig9

Figure 9

Figure 9: Hydrodynamic Modeling of the Interaction of Winds within a Collapsing Turbulent Gas Cloud 