Rotational dynamics of CNCN by p-H2 and o-H2 collision at interstellar temperatures
The rotational dynamics of isocyanogen (CNCN) is studied for its collision with para (p-) and
ortho (o-) hydrogen (H 2) in the temperature range of 1–100 K. These temperatures …
ortho (o-) hydrogen (H 2) in the temperature range of 1–100 K. These temperatures …
The excitation of CNCN in the interstellar medium: hyperfine resolved rate coefficients and non-LTE modelling
D Ndaw, CT Bop, G Dieye, NAB Faye… - Monthly Notices of the …, 2021 - academic.oup.com
The recent detections of CNCN and HNCCN+ are seen as further evidence of the large
abundance of NCCN in the interstellar medium. The accurate determination of the …
abundance of NCCN in the interstellar medium. The accurate determination of the …
Ab initio vibration—rotation coupling constants and the equilibrium geometries of NCCN and CNCN
P Botschwina, J Flügge - Chemical physics letters, 1991 - Elsevier
The equilibrium geometries of NCCN and CNCN were calculated from experimental ground-
state rotational constants and ab initio values for the vibration—rotation coupling constants …
state rotational constants and ab initio values for the vibration—rotation coupling constants …