Author Institution: School of Chemistry, University of Sydney, NSW 2006,; AustraliaHigh level \textit{ab initio} calculations were carried out on the $X^1\Sigma^+_g$, $A^1\Pi_u$, $a^3\Pi_u$, $b^3\Sigma^-_g$, $c^3\Sigma^+_u$ and $d^3\Pi_g$ levels of the C$_2$ radical. Calculations were carried out at the MRCI level with full-valence CASSCF reference wavefunctions and basis sets up to aug-cc-pv6z. The resulting wavefunctions and potential energy surfaces were employed to calculate Einstein coefficients for allowed transitions and intercombination bands. These values were used to model the behaviour of the C$_2$ system in interstellar and circumstellar environments, paying particular attention to the Red Rectangle (HD 44179)
This work focuses on computation of simulated spectra the C2nH family (n = {1, 2,...}) of carbon cha...
The potential energy curves of C2- in its 2 Sigma g+, 2 Pi and 2 Sigma u+ states are constructed by ...
Author Institution:Self-consistent field plus configuration interaction calculations of the electron...
$^{1}$ T. G. Heil and H. F. Schaefer III, J. Chem. Phys. 56, 958 (1972).Author Institution: IBM San ...
S. R. Langhoff: NRC Associate.Author Institution: NASA Ames Research Center NASAAb-initio SCF + CI c...
International audienceThe first electronic states of C$_2$O$^+$ correlating to the first asymptotes ...
Dicarbon (\ce{C2}) is one of the most abundant molecules in space and has been detected in different...
Author Institution: School of Chemistry, University of Sydney, NSW 2006, AustraliaThe $d^{3}\Pi_{g}-...
Context. An accurate analysis of the physical-chemical conditions in the regions of the interstellar...
Calculations at the HFj4-31G level were performed for the C2S2 molecule. The ground state is predict...
Investigating the elusive relationship between our interstellar medium and its assortment of complex...
Author Institution: Department of Chemistry, University of Oslo; Institute of Theoretical Physics, U...
Author Institution: Max Planck Institute of Astrophysics; Physikalisch-Chemisches Institut, Justus-L...
Author Institution: Physics Department, University of New Brunswick$C_{2}H$ is a linear radical foun...
In this paper, the structure and spectroscopic parameters of the C-5 cluster are determined using mu...
This work focuses on computation of simulated spectra the C2nH family (n = {1, 2,...}) of carbon cha...
The potential energy curves of C2- in its 2 Sigma g+, 2 Pi and 2 Sigma u+ states are constructed by ...
Author Institution:Self-consistent field plus configuration interaction calculations of the electron...
$^{1}$ T. G. Heil and H. F. Schaefer III, J. Chem. Phys. 56, 958 (1972).Author Institution: IBM San ...
S. R. Langhoff: NRC Associate.Author Institution: NASA Ames Research Center NASAAb-initio SCF + CI c...
International audienceThe first electronic states of C$_2$O$^+$ correlating to the first asymptotes ...
Dicarbon (\ce{C2}) is one of the most abundant molecules in space and has been detected in different...
Author Institution: School of Chemistry, University of Sydney, NSW 2006, AustraliaThe $d^{3}\Pi_{g}-...
Context. An accurate analysis of the physical-chemical conditions in the regions of the interstellar...
Calculations at the HFj4-31G level were performed for the C2S2 molecule. The ground state is predict...
Investigating the elusive relationship between our interstellar medium and its assortment of complex...
Author Institution: Department of Chemistry, University of Oslo; Institute of Theoretical Physics, U...
Author Institution: Max Planck Institute of Astrophysics; Physikalisch-Chemisches Institut, Justus-L...
Author Institution: Physics Department, University of New Brunswick$C_{2}H$ is a linear radical foun...
In this paper, the structure and spectroscopic parameters of the C-5 cluster are determined using mu...
This work focuses on computation of simulated spectra the C2nH family (n = {1, 2,...}) of carbon cha...
The potential energy curves of C2- in its 2 Sigma g+, 2 Pi and 2 Sigma u+ states are constructed by ...
Author Institution:Self-consistent field plus configuration interaction calculations of the electron...