Figure 6 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

Imaging Magnetically Driven Astrospheres: A Forward Modeling Approach

Authors: Ziqi Wu, Tom Van Doorsselaere, Jiansen He, Hugues Sana, Nicholas Jannsen, Tianhang Chen, Weining Wang, Zheng Sun

Ziqi Wu et al 2026 The Astrophysical Journal Letters 1005 .

Provider: AAS Journals

Caption: Figure 6.

Distribution of the peak positions in the emission spectra after ISM absorption. The positions are given as wavelength shifts δλ (left color bar) and the corresponding Doppler velocity shifts δv (right color bar).

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions