Ethylene in the circumstellar envelope of IRC+10216
Abstract
Ethylene (C2H4) is a symmetric molecule that is best detected using mid-infrared transitions. We report on observations of the 10.5 μm ν7 band using the cryogenic grating spectrograph TEXES. These confirm the previous ethylene detection in the IRC+10216 circumstellar shell. We detect 18 ethylene lines. The lines are both narrow and weak with depths of no more than ~2%. The ethylene lines suggest an excitation temperature of ~80 K.
- Publication:
-
Organic Matter in Space
- Pub Date:
- October 2008
- DOI:
- 10.1017/S1743921308021443
- Bibcode:
- 2008IAUS..251..161H
- Keywords:
-
- Techniques: spectroscopic;
- stars: carbon;
- circumstellar matter;
- ISM: molecules;
- infrared: stars