Evidence for cold-stream to hot-accretion transition as traced by Lyα emission 
from groups and clusters at 2 < z < 3.3

Daddi, E.; Rich, R. M.; Valentino, F.; Jin, S.; Delvecchio, I.; Liu, D.; Strazzullo, V.; Neill, J.; Gobat, R.; Finoguenov, A.; Bournaud, F.; Elbaz, D.; Kalita, B. S.; O’Sullivan, D.; Wang, T.

doi:10.3847/2041-8213/ac531f

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Evidence for cold-stream to hot-accretion transition as traced by Lyα emission from groups and clusters at 2 < z < 3.3

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Liu, D.
MPI for Extraterrestrial Physics, Max Planck Society;

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Daddi, E., Rich, R. M., Valentino, F., Jin, S., Delvecchio, I., Liu, D., et al. (2022). Evidence for cold-stream to hot-accretion transition as traced by Lyα emission from groups and clusters at 2 < z < 3.3. The Astrophysical Journal Letters, 926(2): L21. doi:10.3847/2041-8213/ac531f.

Cite as: https://hdl.handle.net/21.11116/0000-000A-27BE-5

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