Cosmic evolution of black hole spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
<p>Black holes (BHs) are ubiquitous components of the center of most galaxies. In addition to their mass, the BH spin, through its amplitude and orientation, is a key factor in the galaxy formation process, as it controls the radiative efficiency of the accretion disk and relativistic jets. Us...
मुख्य लेखकों: | Peirani, S, Suto, Y, Beckmann, RS, Volonteri, M, Lin, Y-T, Dubois, Y, Yi, SK, Pichon, C, Kraljic, K, Park, M, Devriendt, J, Han, S, Chen, W-H |
---|---|
स्वरूप: | Journal article |
भाषा: | English |
प्रकाशित: |
EDP Sciences
2024
|
समान संसाधन
-
Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations
द्वारा: Volonteri, M, और अन्य
प्रकाशित: (2020) -
Introducing the NEWHORIZON simulation: galaxy properties with resolved internal dynamics across cosmic time
द्वारा: Dubois, Y, और अन्य
प्रकाशित: (2021) -
Population statistics of intermediate-mass black holes in dwarf galaxies using the newhorizon simulation
द्वारा: Beckmann, RS, और अन्य
प्रकाशित: (2023) -
The NewHorizon simulation – to bar or not to bar
द्वारा: Reddish, J, और अन्य
प्रकाशित: (2022) -
On the Origin of Star Formation Quenching of Galaxies in Group Environments Using the NewHorizon Simulation
द्वारा: Jinsu Rhee, और अन्य
प्रकाशित: (2024-01-01)