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Isotopic Ratios in the Disk of HD 163296

  • Authors: Chunhua Qi, David J. Wilner, Catherine C. Espaillat

Chunhua Qi et al 2026 The Astrophysical Journal Letters 997 .

  • Provider: AAS Journals

Caption: Figure 1.

Radial profile (top) and derivative (bottom) of the 13C18O(2–1) integrated intensity toward HD 163296. The derivative profile shows a clear local minimum at ∼0﹩\mathop{.}\limits^{\unicode{x02033}}﹩75, consistent with the location of the sharp CO snowline transition observed in C17O and C18O lines (C. Qi & D. J. Wilner 2024).

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