How galaxies lose their angular momentum

@article{DOnghia2006HowGL,
  title={How galaxies lose their angular momentum},
  author={Elena D’Onghia and Andreas Burkert and Giuseppe Murante and Stephan Munich and Inaf Oat and Oxford and Mpe - Garching},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2006},
  volume={372},
  pages={1525-1530}
}
The processes are investigated by which gas loses its angular momentum during the protogalactic collapse phase, leading to disc galaxies that are too compact with respect to the observations. High-resolution N-body/SPH simulations in a cosmological context are presented including cold gas and dark matter (DM). A halo with quiet merging activity since redshift z ∼ 3.8 and with a high-spin parameter is analysed that should be an ideal candidate for the formation of an extended galactic disc. We… Expand
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