Ethylene in the circumstellar envelope of IRC+10216

7Citations
Citations of this article
11Readers
Mendeley users who have this article in their library.

Abstract

Ethylene (C2H4) is a symmetric molecule that is best detected using mid-infrared transitions. We report on observations of the 10.5 m 7 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. © 2008 International Astronomical Union.

Cite

CITATION STYLE

APA

Hinkle, K. H., Wallace, L., Richter, M. J., & Cernicharo, J. (2008). Ethylene in the circumstellar envelope of IRC+10216. In Proceedings of the International Astronomical Union (Vol. 4, pp. 161–162). https://doi.org/10.1017/S1743921308021443

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free