JOYS+ study of solid state C/C isotope ratios in protostellar envelopes: Observations of CO and CO ice with JWST
arXiv:2409.17237 · doi:10.1051/0004-6361/202451794
Abstract
The carbon isotope ratio is a powerful tool for studying the evolution of stellar systems. Recent detections of CO isotopologues in disks and exoplanet atmospheres pointed towards significant fractionation in these systems. In order to understand the evolution of this quantity, it is crucial to trace the isotope abundance from stellar nurseries to planetary systems. During the protostellar stage the multiple vibrational modes of CO and CO ice provide a unique opportunity to examine the carbon isotope ratio in the solid state. Now with the sensitivity of the \textit{James Webb Space Telescope}, these absorption features have become accessible at high S/N in Solar-mass systems. We quantify the CO/CO and the CO/CO isotope ratios in 17 class 0/I low mass protostars from the CO combination modes (2.70 m and 2.77 m), the CO stretching mode (4.27 m), the CO stretching mode (4.39 m), the CO bending mode (15.2 m), the CO stretching mode (4.67 m) and the CO stretching mode (4.78 m) using JWST observations. We also report a detection of the CO overtone mode at 2.35 m. The CO/CO ratios are in agreement and we find mean ratios of 85 23, 76 12 and 97 17 for the 2.70 m, 4.27 m and the 15.2 m bands, respectively. The main source of uncertainty stem from the error on the band strengths. The CO/CO ratios derived from the 4.67 m bands are consistent, albeit elevated with respect to the CO/CO ratios and we find a mean ratio of 165 52. These findings indicate that ices leave the pre-stellar stage with elevated carbon isotope ratios relative to the interstellar medium and that fractionation becomes significant during the later stages.
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