We report on and discuss the detection of an emission feature at 14.98
mu m from the oxygen-rich, semi-regularly pulsating asymptotic Giant
Branch star R Crateris, a feature which we suggest to be due to the 2(
0)(1) Q-branch of circumstellar CO2. We also suggest a reasonable exci
tation mechanism, which could explain the height, the width and the as
ymmetry of the feature.