Saved in:
| Main Author: | |
|---|---|
| Format: | Recurso digital |
| Language: | |
| Published: |
Zenodo
2026
|
| Online Access: | https://doi.org/10.5281/zenodo.18804799 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Table of Contents:
- Supermassive Black Holes (SMBHs) at the centers of high-z quasars are observed to have grown to masses >= 10^9 Msun by redshifts z=6-7. Recent JWST observations are additionally revealing the existence of central intermediate-mass BHs (10^7 - 10^8 Msun) at even earlier epochs z~10-12; some of which sources have BH mass comparable to the mass of the host galaxy. At the same time, very recent JWST observations have detected a population of normal-mass central SMBHs at z~3-5, with the mean SMBH-to stellar mass ratio consistent with the local relation. The formation of such supermassive (overmassive and normal-mass) BHs at the centers of their host galaxies involves unresolved questions.