X-ray signatures of galactic outflows into the circumgalactic medium

HIGHLIGHTS

• What: It is, however, difficult to determine the main reason for such behaviour in global simulations due to the complex coupling of multiple parameters in the numerical evolution. The total pressure in this model has three components, i.e. thermal (pth ), non-thermal (pnth ), and turbulent (pturb ) pressure. Since the authors aim to study the interaction between a galactic wind and the CGM the authors ignore the detailed modelling of the wind collimation during the launch of the wind and assume it is collimated to an opening angle. To understand the impact of the different energy injection . . .
  

   

  

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