High-redshift Halo–Galaxy Connection via Constrained Simulations
The evolution of halos with masses around M _h ≈ 10 ^11 M _⊙ and M _h ≈ 10 ^12 M _⊙ at redshifts z > 9 is examined using constrained N -body simulations. The average specific mass accretion rates, ${\dot{M}}_{{\rm{h}}}/{M}_{{\rm{h}}}$ , exhibit minimal mass dependence and generally agree with exi...
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| Format: | Article |
| Language: | English |
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IOP Publishing
2024-01-01
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| Series: | The Astrophysical Journal |
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| Online Access: | https://doi.org/10.3847/1538-4357/ad702c |