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Using Scattered Near-infrared Light to Map Water Ice in Prestellar Cores with SPHEREx

  • Authors: Tamojeet Roychowdhury, Jennifer B. Bergner, Jens Kauffmann, Thushara G. S. Pillai, Silvia Spezzano

Tamojeet Roychowdhury et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 3.

Top row: averaged radial profile of ice absorption depth τice (and ±1σ uncertainty band—upper error including an additional 10% for the unknown τice correction factor) observed in the four cores. The lower-density cores on the left (L1512 and L260) have a monotonically decreasing ice depth from the center outward. The higher-density cores on the right (CrA 151 and L1544) show a drop in ice absorption depth at the center. Bottom row: model-derived light profile and ice absorption profile as a function of radius for the prestellar core as described in Section 3.2—continuum profile for varying densities (left), ice absorption profile for varying densities (middle), and ice absorption profile for varying ice opacities (right).

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