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High Water D/H Ratio of the Interstellar Object 3I/ATLAS is Consistent with a Low-metallicity Origin

  • Authors: Kenji Furuya, Martin Cordiner, Dominique Bockelée-Morvan, Dennis Bodewits, Colin Orion Chandler, Maria N. Drozdovskaya, Nathan X. Roth, Geronimo Villanueva

Kenji Furuya et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

Temporal evolution of selected species and D/H ratios during the cloud (top panels) and core stages (lower panels). Panels (a) and (e) show the abundances of selected species during the cloud and core stages, respectively. Solid, dashed, and dotted lines denote models with Z = 1, 0.5, and 0.2, respectively. The remaining panels show the temporal evolution of the D/H ratios and the H2 OPR for Z = 1 (b), (f), Z = 0.5 (c), (g), and Z = 0.2 (d), (h). In all panels, time is normalized by τfreeze for the corresponding density and metallicity.

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