José L. Alonso, Jean-Claude Guillemin, Carmen Barrientos, Antonio Largo, José Cernicharo, Carlos Cabezas, Spanish National Research Council (CSIC), Universidad de Valladolid [Valladolid] (UVa), Institut des Sciences Chimiques de Rennes (ISCR), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Ecole Nationale Supérieure de Chimie de Rennes (ENSCR)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013) / ERC-2013-SyG [610256 NANOCOSMOS], Ministerio de Economia y Competitividad of Spain [CTQ 2013-40717-P, CTQ 2013-76393-P, AYA2017-87515-P], Junta de Castilla y Leon [VA175U13, VA010G18, VA077U13], Centre National d'Etudes Spatiales (CNES), Program PCMI (INSU-CNRS), Ministerio de Economia y Competitividad of Spain (Consolider-Ingenio 2010) [CSD2009-00038], European Project: 610256,EC:FP7:ERC,ERC-2013-SyG,NANOCOSMOS(2014), Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC)-Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Ecole Nationale Supérieure de Chimie de Rennes (ENSCR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA), European Commission, Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Junta de Castilla y León, Centre National D'Etudes Spatiales (France), and Centre National de la Recherche Scientifique (France)
Producción Científica, The metallic cyanoacetylides LiC3N, NaC3N, MgC3N, and CaC3N have been investigated by combined spectroscopy measurements and theoretical calculations. The theoretical calculations predict for the four species that the linear isomer with the formula MCCCN (M = Li, Na, Mg, and Ca) is the most stable one. We used laser ablation molecular beam Fourier transform microwave (FTMW) spectroscopy to synthesize these species by the reaction of metal vapors, produced by laser ablation, and 3-bromo-2-propynenitrile (BrCCCN). Pure rotational spectra were observed by FTMW spectroscopy in the 2–18 GHz frequency region only for LiCCCN and NaCCCN, while no spectral signatures for MgCCCN and CaCCCN could be detected. Finally, we have searched for LiCCCN and NaCCCN species toward the carbon-rich evolved star IRC +10 216, but only upper limits to their abundances have been obtained., Consejo Europeo de Investigación a través del VII Programa Marco de Investigación y Desarrollo (grant 610256 NANOCOSMOS), Ministerio de Economía, Industria y Competitividad (grants CTQ 2013-40717-P / CTQ 2013-76393-P / AYA2017-87515-P / Consolider-Ingenio 2010 CSD2009-00038), Junta de Castilla y León (grants VA175U13 / VA010G18 / VA077U13)