Wide-angle protostellar outflows driven by narrow jets in stratified cores

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SUMMARY

    Conversely, a magnetic_field in the ambient medium would tend to resist against the sideways shell expansion. A significant reduction in shell width compared to the hydrodynamical case A118, page 16 of 19 n=2, adopted in the present work, the maximum reduction in shell width due to ambient magnetic_field is only 25%, therefore, the predicted cavity shapes and dynamics should remain valid. Each large H2 bowshock, produced by a major jet pulse, is seen to connect to a separate CO shell at the flow base, nested inside the main cavity (see Fig 2 in . . .

     

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