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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 3.

The reddening-to-extinction ratio fG as a function of E(B − V), derived using the extinction curve from K. D. Gordon et al. (2023) for R0 = 2.60 (RV = 3.06), assuming stellar parameters typical for the young giants: [Fe/H] = 0 dex; Teff = 5100 K, logg = 1.5 dex.

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