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The Flare and Spiral Structure of the Milky Way’s Disk as Traced by Young Giant Stars

  • Authors: E. Poggio, R. Drimmel, S. Khanna, R. Andrae, M. G. Lattanzi

E. Poggio et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure 4.

Examples of fitted vertical distributions in individual cells. Each panel corresponds to a different cell in the XY-plane. For a given cell, the black points show the observed star counts along the vertical coordinate ﹩Z^{\prime} =Z-{Z}_{{\rm{m}}{\rm{e}}{\rm{d}}}﹩, where Zmed is the median Z of the stars in that cell. The red dashed line shows the best-fit model obtained in this work. For illustrative purposes only, the gray-dashed line shows the same best-fit model, but without accounting for the survey selection function and extinction.

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