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Erratum: "Three-dimensional Simulations of Magnetospheric Accretion in a T Tauri Star: Accretion and Wind Structures Just Around the Star" (2022, ApJ, 941, 73)

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Published 2023 March 29 • © 2023. The Author(s). Published by the American Astronomical Society.
, , Citation Shinsuke Takasao et al 2023 ApJ 946 57 DOI 10.3847/1538-4357/acc39b

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takasao@astro-osaka.jp

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1 Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan; takasao@astro-osaka.jp

2 Astronomical Institute, Tohoku University, Sendai, Miyagi 980-8578, Japan

3 Center for Computational Astrophysics, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan

4 School of Arts & Sciences, The University of Tokyo, 3-8-1, Komaba, Meguro, Tokyo, 153-8902, Japan

5 Department of Astronomy, The University of Tokyo, 7-3-1, Hongo, Bunkyo, Tokyo, 113-0033, Japan

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  1. Received 2023 March 8
  2. Accepted 2023 March 12
  3. Published

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0004-637X/946/1/57

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Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

We correct the description of the cooling function in Section 2.4 of the published article. The temperature range in which the cooling term is activated was Tdisk,ref < T, not Tdisk,ref < T < 0.3 T*. The radiative cooling timescale at each radius is set to 20% of one orbital period, not to 40%. In this sense, the results of the published article may be considered a case in which radiative cooling is efficient. We will investigate the impact of the thermal structure on the accretion and ejection processes in future papers.

10.3847/1538-4357/acc39b