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An Analytic Model for Stellar Metallicity Gradient Residuals in Cold, Phase-mixed Galactic Disks

  • Authors: Shaunak Modak, Zoe Hackshaw, Keith Hawkins

Shaunak Modak et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

Absolute metallicity-residual distributions produced by formation and migration processes (panel (a)), epicyclic blurring (panel (b)), and the combination of both effects (panel (c)). Different colors indicate different epicyclic amplitudes, while different line styles indicate different amounts of scatter from formation and migration. To produce these curves, we have used mR = −0.0678 dex kpc–1 as measured for μ = [Fe/H] by Z. Hackshaw et al. (2024).

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