The effects of galaxy shape and rotation on the X-ray haloes of early-type galaxies – II. Numerical simulations

@article{Negri2014TheEO,
  title={The effects of galaxy shape and rotation on the X-ray haloes of early-type galaxies – II. Numerical simulations},
  author={Andrea Negri and Silvia Posacki and Silvia Pellegrini and Luca Ciotti},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2014},
  volume={445},
  pages={1351-1369}
}
By means of high resolution 2D hydrodynamical simulations, we study the evolution of the hot ISM for a large set of early-type galaxy models, characterized by various degrees of flattening and internal rotation. The galaxies are described by state-of-the-art axisymmetric two-component models, tailored to reproduce real systems; the dark matter haloes follow the Navarro-Frenk-White or the Einasto profile. The gas is produced by the evolving stars, and heated by Type Ia SNe. We find that, in… 
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