Single-dish observations and non-LTE analysis of CH3OH, HCN, and CO line emission in the Oort cloud comet C/2017 K2 (PANSTARRS)

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ID: 317080
2026
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Abstract
Abstract We present pre-perihelion observations of methanol, carbon monoxide, and hydrogen cyanide in the Oort cloud comet C/2017 K2 (PANSTARRS), performed with the APEX 12-m and Onsala 20-m telescopes from April to July 2022. As the comet’s heliocentric distance decreased from 3.4 to 2.7 AU, CH3OH line intensities increased substantially (by factors of 1.1–4.0), with the most pronounced enhancement in lines with upper-level energies Eu > 40 K. In contrast, the brightness of the CO and HCN lines remained constant. We estimate the best-fit gas kinetic temperatures Tgas > 100 K and water production rate of $Q_{\rm H_2O}=(3-10)\times 10^{28}$ s−1. The derived methanol-to-water abundance ratio ≈0.01 − 0.04, depending on the observed period. Our results demonstrate that non-LTE effects are dominant in the coma and must be accounted for to accurately derive molecular production rates. We also report weak non-thermal excitation, including potential maser activity in the CH3OH 80 − 71 line.
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Authors M. S. Kirsanova, Ya. N. Pavlyuchenkov, A O H Olofsson, M S Lerner
Journal monthly notices of the royal astronomical society
Year 2026
DOI
10.1093/mnras/stag1086
URL
https://doi.org/10.1093/mnras/stag1086
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