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Mapping Interstellar Ice Inventory toward Class 0 Protostars in Star-forming Region Orion A with JWST Data

  • Authors: Igor Petrashkevich, Yaroslav Pavlyuchenkov, Anna Punanova, Maksim Ozhiganov, Ruslan Nakibov, Varvara Karteyeva, Svetlana Salii, Andrej Sobolev, Mikhail Medvedev, Anton Vasyunin

Igor Petrashkevich et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 6.

Optical depth spectra toward the ALMA continuum intensity peak of the sources. The red line shows the best fit for each spectrum, and the black line shows the optical depth spectrum. The R2 of the fits is shown in the lower right corners. Left panels: Gaussian fits of 13CO2, OCN, CO, and OCS. Right panels: colored lines show the components of the laboratory spectra of H2CO:H2O (blue), H2O (green), NH﹩{}_{4}^{+}﹩ (15 K, purple), H2O:CO:CO2 (orange), and NH﹩{}_{4}^{+}﹩(120 K, cyan).

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