This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

Chemistry of the Organic-Rich Hot Core G327.3–0.6

, , , , and

© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation E. Gibb et al 2000 ApJ 545 309 DOI 10.1086/317805

0004-637X/545/1/309

Abstract

We present gas-phase abundances of species found in the organic-rich hot core G327.3-0.6. The data were taken with the Swedish-ESO Submillimetre Telescope (SEST). The 1-3 mm spectrum of this source is dominated by emission features of nitrile species and saturated organics, with abundances greater than those found in many other hot cores, including Sgr B2 and OMC-1. Population diagram analysis indicates that many species (CH3CN, C2H3CN, C2H5CN, CH3OH, etc.) have hot components that originate in a compact (~2'') region. Gas-phase chemical models cannot reproduce the high abundances of these molecules found in hot cores, and we suggest that they originate from processing and evaporation of icy grain mantle material. In addition, we report the first detection of vibrationally excited ethyl cyanide and the first detection of methyl mercaptan (CH3SH) outside the Galactic center.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/317805