Yoshimine et al. 1973

Yoshimine, M., S. Green, and P. Thaddeus, 1973: Oscillator strengths for the X¹Σ⁺—A¹Π system of CH⁺. Astrophys. J., 183, 899-902.

Oscillator strengths for the X¹Σ⁺—A¹Π system of CH⁺ have been computed to an estimated accuracy of 10 percent from ab initio wave functions. The f_v'v" values for the two strongest interstellar lines, λlambda$4232 and 3957, are founbd to be, respectively, f₀₀ = 6.45×10^-3 and f₁₀ = 4.31×10^-3.

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Yoshimine, M., Green, S., and Thaddeus, P.: Oscillator strengths for the X¹Σ⁺—A¹Π system of CH⁺, Astrophys. J., 183, 899-902, 1973.

Yoshimine, M., S. Green, and P. Thaddeus (1973), Oscillator strengths for the X¹Σ⁺—A¹Π system of CH⁺, Astrophys. J., 183, 899-902.

Yoshimine, M., S. Green, and P. Thaddeus, 1973: Oscillator strengths for the X¹Σ⁺—A¹Π system of CH⁺. Astrophys. J., 183, 899-902.

Yoshimine, M., Green, S., & Thaddeus, P. 1973, Astrophys. J., 183, 899.

Yoshimine M, Green S, Thaddeus P. Oscillator strengths for the X¹Σ⁺—A¹Π system of CH⁺, Astrophys J 1973;183:899-902.

M. Yoshimine, S. Green, P. Thaddeus, Astrophys. J. 183, 899-902 (1973).