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Large-scale Spiral Structure of the Milky Way Traced by Young Classical Cepheids

  • Authors: Z. H. Lin, C. J. Hao, D. J. Liu, Y. J. Li, J. J. Li, Y. W. Dong, Y. X. He, Jarken Esimbek

Z. H. Lin et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

Spatial and extinction distributions of the classical Cepheid sample. Red and blue points represent subsamples A and B, respectively. The top left panel shows the distribution in the Galactic (X−Y) plane. The top right and bottom left panels show the vertical height (Z) as a function of Galactocentric radius (R) and heliocentric distance (d), respectively. The bottom right panel shows the W1-band extinction, (AW1), as a function of d.

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