Identification of solid N2O in interstellar ices using open JWST data
V. Karteyeva, R. Nakibov, I. Petrashkevich, M. Medvedev, A. Vasyunin

TL;DR
This study uses JWST data and laboratory spectra to successfully identify solid N2O in interstellar ices around protostars, revealing its formation environment and abundance.
Contribution
First secure detection of solid N2O in interstellar ices using JWST spectra and laboratory analogs, with insights into its formation and abundance.
Findings
N2O identified in 16 protostars
N2O abundance estimated at 0.2-2.1% relative to CO
N2O forms mainly in the apolar ice layer
Abstract
Context. There are only six molecules containing N-O bond that are detected in gaseous phase in interstellar medium. One of those is nitrous oxide (N2O), which was searched for but not found in solid form from as early as Infrared Space Observatory (ISO) mission was launched. The observational capabilities of James Webb Space Telescope (JWST) present a possibility to identify solid interstellar N2O. Aims. We aim to identify nitrous oxide in open JWST spectra of interstellar ices towards a sample of Class 0, 0/I and flat protostars using the relevant laboratory mixtures of N2O-bearing interstellar ice analogues. Methods. A set of laboratory infrared transmission spectra was obtained for the following mixtures: N2O:CO2=1:20, N2O:CO=1:20, N2O:N2=1:20, N2O:CO2:CO=1:15:5, N2O:CO2:N2=1:15:13 at 10-23 K. A search for N2O in JWST NIRSpec spectra towards 50 protostars was performed by…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
