Issue |
A&A
Volume 668, December 2022
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201628955e | |
Published online | 09 December 2022 |
Evolution of protoplanetary discs with magnetically driven disc winds (Corrigendum)
1
School of Arts & Sciences, University of Tokyo,
3-8-1, Komaba, Meguro,
Tokyo
153-8902, Japan
e-mail: stakeru@ea.c.u-tokyo.ac.jp
2
Department of Physics, Nagoya University,
Nagoya, Aichi
464-8602, Japan
3
Laboratoire Lagrange, Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS Bvd de l’Observatoire,
CS 34229,
06304
Nice Cedex 4, France
4
Division of Theoretical Astronomy, National Astronomical Observatory of Japan,
2-21-1, Osawa, Mitaka,
Tokyo
181-8588, Japan
5
Institut Universitaire de France,
103 bd Saint Michel,
75005
Paris, France
Key words: accretion / accretion disks / ISM: jets and outflows / magnetohydrodynamics (MHD) / protoplanetary disks / stars: winds / outflows / errata / addenda
In the last paragraph of Sect. 2.5 of the original paper, the treatment of the boundary condition was incorrectly described. In the original paper, we stated that was imposed at the inner and outer boundaries, r = rin = 0.01 au and = rout = 104 au, and that this condition corresponds to the zero-torque boundary condition. However, this statement and explanation were incorrect. The actual boundary condition implemented in our calculations was to impose
at r = rin and = rout.
This is consistent with the zero-torque boundary condition, (
for a constant
and
; see Eqs. (10) and (A.5)) → 0 at the centre, r → 0. The physical meaning of
at r = rin and = rout is to impose a constant mass accretion rate induced by the rϕ stress for a constant
and
(Eq. (33)) across the boundary. All of the results presented in the original paper remain unchanged.
© T. K. Suzuki et al. 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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