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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 7.

Peak-intensity maps for lines of sight with different orientations and averaged ISM velocities. From top to bottom, the rows show results with ϕ = 45,  90,  135°, where ϕ is the angle between the upwind direction and the line of sight. From left to right, the columns show results with ΔV = −100, ​​​​​​−30,  0, 30,  100 km s−1.

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