High-resolution [O I] line spectral mapping of TW Hya supportive of magnetothermal wind

Min Fang (Creator)
Lile Wang (Creator)
Gregory J. Herczeg (Creator)
J. Hashimoto (Creator)
Ziyan Xu (Creator)
Ahmad Nemer (Creator)
Ilaria Pascucci (Creator)
Sebastiaan Haffert (Creator)
Yuhiko Aoyama (Creator)

Dataset

Description

The fit files are the 2D images of the [O I] 6300 and He I 6678 and their uncertainties of TW Hya with the PSF images near the two lines.

Date made available	2023
Publisher	figshare

DOI
10.6084/m9.figshare.21906306.v1

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Creative Commons Attribution 4.0 International

High-resolution [O I] line spectral mapping of TW Hya supportive of a magnetothermal wind
Fang, M., Wang, L., Herczeg, G. J., Hashimoto, J., Xu, Z., Nemer, A., Pascucci, I., Haffert, S. Y. & Aoyama, Y., Aug 2023, In: Nature Astronomy. 7, 8, p. 905-912 8 p.
Research output: Contribution to journal › Article › peer-review
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