$z\sim2$ dual AGN host galaxies are disky: stellar kinematics in the ASTRID Simulation
We study dual AGN host galaxy morphologies at $z=2$ using the ASTRID simulation, selecting black hole (BH) pairs with small separation ($\Delta r<30\rm{kpc}$), high mass ($M_{\text{BH,12}}>10^7M_\odot$), and luminosity ($L_{\text{bol,12}}>10^{43}\rm{erg/s}$). We kinematically decompose (using MORDOR...
Furkejuvvon:
| Váldodahkkit: | , , , , , , , , |
|---|---|
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Maynooth Academic Publishing
2024-10-01
|
| Ráidu: | The Open Journal of Astrophysics |
| Liŋkkat: | https://doi.org/10.33232/001c.124451 |
| Fáddágilkorat: |
Eai fáddágilkorat, Lasit vuosttaš fáddágilkora!
|