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Cyclopropenylidenes: From Interstellar Space to an Isolated Derivative in the Laboratory
Author(s) -
Vincent Lavallo,
Yves Canac,
B. Donnadieu,
Wolfgang W. Schoeller,
Guy Bertrand
Publication year - 2006
Publication title -
science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 12.556
H-Index - 1186
eISSN - 1095-9203
pISSN - 0036-8075
DOI - 10.1126/science.1126675
Subject(s) - carbene , heteroatom , chemistry , molecule , derivative (finance) , carbon fibers , singlet state , crystallography , interstellar medium , computational chemistry , ring (chemistry) , materials science , physics , organic chemistry , astrophysics , atomic physics , galaxy , composite number , financial economics , economics , composite material , excited state , catalysis
Like many of the molecular species that have been detected in the interstellar medium, the singlet carbene cyclopropenylidene (C3 H2 ) has been presumed to be too unstable to isolate in the laboratory. However, by appending π-electron–donating amino groups to the triangular skeleton, we prepared a cyclopropenylidene derivative that is stable at room temperature. In contrast to previously isolated carbenes, this compound does not require a heteroatom adjacent to the electron-deficient carbon to confer stability. Despite the presence of amino groups, the geometric parameters of the cyclic skeleton, revealed by x-ray crystallography, are only slightly perturbed relative to those of the calculated structure of unsubstituted cyclopropenylidene. Stable cyclopropenylidene derivatives might thus serve as models for a better understanding of the formation of carbon-bearing molecules in the interstellar medium.

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