OBSERVATIONS. “We predict that these DCBHs will evolve to form the population of faint quasars observed at z ≈ 6. This population will be within the reach of the James Webb Space Telescope, which will be able to provide stringent constraints on their number densities that will be directly comparable to our results.” (DCBH = direct-collapse black holes).
https://www.nature.com/articles/s41586-019-0873-4
linkedin post 2022-06-29 05:12:48
Nigel Fleming
September 21, 2022