Dataset for 'Magnetic Pressure Dominance Stabilizes AGN Disks Against Gravitational Instability'
Abstract
This deposit contains the data shown in the figures in the journal article, 'Magnetic Pressure Dominance Stabilizes AGN Disks Against Gravitational Instability (arXiv:2508.16842).' General formatting information: Each column has a descriptive header. In filenames, b25 refers to simulations with initial beta = 1e2.5; b4 refers to simulations with initial beta = 1e4; q1 refers to simulations with initial Q = 1.0; q10 refers to simulations with initial Q = 10.0. MHD/pure MHD refers to simulations performed without self-gravity. There are 34 total files for the nine figures as follows: Fig. 1 & 2: b25_q1_stresses.txt, b25_q10_stresses.txt, vol_avg_stresses_beta_1e2_5_pure_MHD.txt, b4_q1_stresses.txt, b4_q10_stresses.txt,vol_avg_stresses_beta_1e4_pure_MHD.txt Fig. 3: b25_q1_mag_press.txt, b25_q10_mag_press.txt, b25_MHD_mag_press.txt, b4_q1_mag_press.txt, b4_q10_mag_press.txt, b4_MHD_mag_press.txt Fig. 4: hor_avg_beta_b25_q1.txt, hor_avg_beta_b25_q10.txt, hor_avg_beta_b25_MHD.txt Fig. 5: hor_avg_beta_b4_q1.txt, hor_avg_beta_b4_q10.txt, hor_avg_beta_b4_MHD.txt Fig. 6: hor_avg_rho_b25_q1.txt, hor_avg_rho_b25_q10.txt, hor_avg_rho_beta_1e2_5_MHD.txt, hor_avg_rho_b4_q1.txt, hor_avg_rho_b4_q10.txt, hor_avg_rho_beta_1e4_MHD.txt Fig. 7: density_vert_slice_* Fig. 8: Q_realized_b25_q1.txt, Q_realized_b4_q1.txt Fig. 9: Q_realized_b25_q10.txt, Q_realized_b4_q10.txt
Fields of Study & Subjects
Astrophysical Phenomena and Observations
Galaxies: Formation
Evolution
Phenomena
Astrophysics and Star Formation Studies
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 27 January 2026
- Document type
- Dataset