High-redshift Halo–Galaxy Connection via Constrained Simulations
Abstract
The evolution of halos with masses around M h ≈ 1011 M ⊙ and M h ≈ 1012 M ⊙ at redshifts z > 9 is examined using constrained N-body simulations. The average specific mass accretion rates,
- Publication:
-
The Astrophysical Journal
- Pub Date:
- October 2024
- DOI:
- 10.3847/1538-4357/ad702c
- arXiv:
- arXiv:2402.18942
- Bibcode:
- 2024ApJ...974...27N
- Keywords:
-
- High-redshift galaxies;
- Galaxies;
- Star formation;
- 734;
- 573;
- 1569;
- Astrophysics - Astrophysics of Galaxies;
- Astrophysics - Cosmology and Nongalactic Astrophysics
- E-Print:
- Accepted for publication in the ApJ. 13 pages, 6 figures