Effect of multi-dust species on the inner rim of magnetized protoplanetary disks

Home

All issues

Volume 701 (September 2025)

A&A, 701 (2025) A259

Full HTML

Open Access

Table 3

Overview of the magnetized disk models.

Model	B_z [G]	β_z at 1 au	T_∆	$R_{r i m}^{i n}$ $R^\mathrm{in}_{\rm rim}$	$R_{r i m}^{o u t}$ $R^{\rm out}_{\rm rim}$	∆R_rim	τ_z = 1 at $R_{r i m}^{o u t}$ $R^{\rm out}_{\rm rim}$ [rad]
M001	0.01	2.29 · 10⁶	100K	0.33 au	0.52 au	0.19 au	0.085
M01	0.1	2.29 · 10⁴	100K	0.33 au	0.52 au	0.19 au	0.085
M03	0.3	2.51 · 10³	100K	0.33 au	0.52 au	0.19 au	0.085
M001_S	0.01	2.29 · 10⁶	100K	0.42 au	0.54 au	0.12 au	0.082
M001_S_TC	0.01	2.29 · 10⁶	100K	0.26 au	0.40 au	0.14 au	0.073
MZ_S	10⁻⁴	1.52 · 10¹⁰	100K	0.42 au	0.54 au	0.12 au	0.082
MZ	10⁻⁴	1.52 · 10¹⁰	100K	0.33 au	0.52 au	0.19 au	0.085
MZ_TD50	10⁻⁴	1.52 · 10¹⁰	50 K	0.36 au	0.56 au	0.20 au	0.093

Notes. From left to right: model name, the midplane vertical magnetic field strength at 1 au, and the plasma beta of the vertical magnetic field at the midplane at 1 au.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.