Pre-perihelion observations of comet C/2017 K2 show increasing CH3OH line intensities with decreasing heliocentric distance, non-LTE dominated excitation, Tgas >100 K, and CH3OH/H2O ratio of 0.01-0.04.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
years
2026 2verdicts
UNVERDICTED 2representative citing papers
APEX 1.3 mm observations of RCW120 S2 detect COMs including CH3OH, CH3CHO, CH3OCHO and CH3OCH3, reveal a radially stratified envelope, and show modest abundance mismatches with hot-core chemical models attributed to unresolved filling factor.
citing papers explorer
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Single-dish observations and non-LTE analysis of CH3OH, HCN, and CO line emission in the Oort cloud comet C/2017 K2 (PANSTARRS)
Pre-perihelion observations of comet C/2017 K2 show increasing CH3OH line intensities with decreasing heliocentric distance, non-LTE dominated excitation, Tgas >100 K, and CH3OH/H2O ratio of 0.01-0.04.
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Complex organic molecules in the young hot core RCW 120 S2
APEX 1.3 mm observations of RCW120 S2 detect COMs including CH3OH, CH3CHO, CH3OCHO and CH3OCH3, reveal a radially stratified envelope, and show modest abundance mismatches with hot-core chemical models attributed to unresolved filling factor.