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Mapping the WISPIT 2 Planet-hosting Cavity at Sub-Hill-radius Scales

  • Authors: Myriam Benisty, Stefano Facchini, Richard Teague, Francesco Zagaria, Pietro Curone, Viviana Pezzotta, Jaehan Bae, Gabriele Cugno, Daniel J. Price

Myriam Benisty et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 5.

Zoomed-in 12CO J = 3−2 channel maps. Contours are 3σ, 6σ and 10σ. The isovelocity contours are calculated with a flat surface. The planet locations are marked with white dots. The beam is given in the bottom-right corner, while the velocity of the channel is provided in the bottom-left corner. Figure F5 shows the channel maps over the full extent of the disk.

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