Journal
PHYSICAL CHEMISTRY CHEMICAL PHYSICS
Volume 5, Issue 16, Pages 3337-3348Publisher
ROYAL SOC CHEMISTRY
DOI: 10.1039/b303753n
Keywords
-
Ask authors/readers for more resources
Over the past two decades, the identification and characterisation of interstellar molecules has often benefitted from a fruitful interplay between theoretical chemistry, laboratory spectroscopy and ( radio) astronomy. The article reports on various examples of this sort, concentrating on carbon chains which represent the most prominent structural motif among currently known interstellar molecules. Results of large-scale coupled cluster calculations are reported for cyanopolyynes (HC2n+1N) up to n = 5, the corresponding radicals C2n+1N, linear silicon carbides ( SiCn), carbon-sulfur and pure carbon chains. Throughout, detailed comparison with experimental data is made wherever possible.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available