Cabezas Carlos, Barrientos Carmen, Largo Antonio, Guillemin Jean-Claude, Cernicharo José, Peña Isabel, Alonso José L
Grupo de Espectroscopia Molecular (GEM), Edificio Quifima, Laboratorios de Espectroscopia y Bioespectroscopia, Unidad Asociada CSIC, Parque Científico Uva, Universidad de Valladolid, Paseo de Belén 5, 47011 Valladolid, Spain.
Departamento de Química Física y Química Inorgánica, Facultad de Ciencias, Universidad de Valladolid, Campus Miguel Delibes, Paseo de Belén 7, 47011 Valladolid, Spain.
J Chem Phys. 2014 Sep 14;141(10):104305. doi: 10.1063/1.4894501.
Combined spectroscopy measurements and theoretical calculations bring to light a first investigation of a metallic cyanoacetylide, AlC3N, using laser ablation molecular beam Fourier transform microwave spectroscopy. This molecule was synthesized in a supersonic expansion by the reaction of aluminum vapour with C3N, produced from solid aluminum rods and BrCCCN in a newly constructed ablation-heating nozzle device. A set of accurate rotational and (27)Al and (14)N nuclear quadrupole coupling constants have been determined from the analysis of the rotational spectrum and compared with those predicted in a high-level ab initio study, conducting to the assignment of the observed species to linear AlCCCN. We have searched for this species towards the carbon-rich evolved star IRC + 10216 but only an upper limit to its abundance has been obtained.
结合光谱测量和理论计算,首次利用激光烧蚀分子束傅里叶变换微波光谱对金属氰基乙炔化物AlC₃N进行了研究。该分子是在一个新建的烧蚀加热喷嘴装置中,通过铝蒸汽与由实心铝棒和BrCCCN反应生成的C₃N在超声速膨胀中合成的。通过对转动光谱的分析,确定了一组精确的转动常数以及(²⁷)Al和(¹⁴)N核四极耦合常数,并与高水平从头算研究预测的结果进行了比较,从而将观测到的物种归属为线性AlCCCN。我们在富含碳的演化恒星IRC + 10216中搜索了该物种,但仅获得了其丰度的上限。