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The physical origins of gas in the circumgalactic medium using observationally motivated TNG50 mocks

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Casavecchia,  Benedetta
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Weng, S., Peroux, C., Ramesh, R., Nelson, D., Sadler, E. M., Zwaan, M., et al. (2023). The physical origins of gas in the circumgalactic medium using observationally motivated TNG50 mocks. Monthly Notices of the Royal Astronomical Society, 527(2), 3494-3516. doi:10.1093/mnras/stad3426.


Cite as: https://hdl.handle.net/21.11116/0000-000E-6DBE-3
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