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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 6.

RADMC-3D derived ice absorption map for Top left: the fiducial cloud for a constant ηice = 40%, same as Figure 4, for comparison. Top right: a cloud illuminated at 30∘ to the LoS, the source of illumination being in the top part of the image. Middle left: a cloud where central regions have grain sizes reaching up to 100 μm instead of 5 μm. Middle right: a cloud where ice formation primarily happens at densities ﹩{n}_{{{\rm{H}}}_{2}}\,\geqslant \,1{0}^{4}﹩ cm−3. Bottom left: a cloud where ice density becomes constant/saturates above gas densities of ﹩{n}_{{{\rm{H}}}_{2}}\,\geqslant \,1{0}^{4}﹩ cm−3, and does not scale with the increasing gas/dust density. Bottom right: a cloud where ice changes from being pure H2O, to a mix of a 3:1 mix of CO and H2O ice, at densities ﹩{n}_{{{\rm{H}}}_{2}}\,\geqslant \,1{0}^{4}﹩ cm−3.

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