Green 1980

Green, S., 1980: Theoretical microwave spectral constants for C₂N, C₂N², and C₃H. Astrophys. J., 240, 962-967, doi:10.1086/158310.

Theoretical microwave spectral constants have been computed for C₂N, C₃H, and C₂N⁺. For C₂N these are compared with values obtained from optical data. Calculated hyperfine constants are also presented for HNC, DNC, and HCNH⁺. The possibility of observing these species in dense interstellar clouds is discussed.

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Green, S.: Theoretical microwave spectral constants for C₂N, C₂N², and C₃H, Astrophys. J., 240, 962-967, doi:10.1086/158310, 1980.

Green, S. (1980), Theoretical microwave spectral constants for C₂N, C₂N², and C₃H, Astrophys. J., 240, 962-967, doi:10.1086/158310.

Green, S., 1980: Theoretical microwave spectral constants for C₂N, C₂N², and C₃H. Astrophys. J., 240, 962-967, doi:10.1086/158310.

Green, S. 1980, Astrophys. J., 240, 962, doi:10.1086/158310.

Green S. Theoretical microwave spectral constants for C₂N, C₂N², and C₃H, Astrophys J 1980;240:962-967. doi:10.1086/158310.

S. Green, Astrophys. J. 240, 962-967, doi:10.1086/158310 (1980).