Radiation and Magnetic Pressure Support in Accretion Disks Around Supermassive Black Holes and the Physical Origin of the Extreme-ultraviolet to Soft X-Ray Spectrum
We present the results of four 3D radiation magnetohydrodynamic simulations of accretion disks around a 10 ^8 solar mass black hole, which produce the far-ultraviolet spectrum peak and demonstrate a robust physical mechanism for producing the extreme-ultraviolet to soft X-ray power-law continuum com...
Saved in:
Main Authors: | Yan-Fei Jiang, Omer Blaes, Ish Kaul, Lizhong Zhang |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/addecb |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Accretion of Active Galactic Nucleus Stars Under the Influence of Disk Geometry
by: Yi-Xian Chen, et al.
Published: (2025-01-01) -
Cyclic Zoom: Multiscale GRMHD Modeling of Black Hole Accretion and Feedback
by: Minghao Guo, et al.
Published: (2025-01-01) -
Iron-corrected Single-epoch Black Hole Masses of DESI Quasars at Low Redshift
by: Zhiwei Pan, et al.
Published: (2025-01-01) -
J1406+0102: A Dust-obscured Galaxy Hiding a Super-Eddington Accretion System with Bright Radio Emission
by: Hikaru Fukuchi, et al.
Published: (2025-01-01) -
Spectroastrometry and Reverberation Mapping of Active Galactic Nuclei. II. Measuring Geometric Distances and Black Hole Masses of Four Nearby Quasars
by: Yan-Rong Li, et al.
Published: (2025-01-01)