Green and Chapman 1978

Green, S., and S. Chapman, 1978: Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC₃N. Astrophys. J. Supp. Series, 37, 169-194, doi:10.1086/190523.

Rates for excitation of CO, CS, OCS, and HC₃ N by collisions with He atoms and H₂ molecules are presented. These have been obtained from extensive theoretical calculations using methods of known reliability. In general, rates necessary for modeling interstellar molecular clouds with kinetic temperatures to 100 K have been included. Methods for fitting these rates in more compact form are discussed.

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Green, S., and Chapman, S.: Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC₃N, Astrophys. J. Supp. Series, 37, 169-194, doi:10.1086/190523, 1978.

Green, S., and S. Chapman (1978), Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC₃N, Astrophys. J. Supp. Series, 37, 169-194, doi:10.1086/190523.

Green, S., and S. Chapman, 1978: Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC₃N. Astrophys. J. Supp. Series, 37, 169-194, doi:10.1086/190523.

Green, S., & Chapman, S. 1978, Astrophys. J. Supp. Series, 37, 169, doi:10.1086/190523.

Green S, Chapman S. Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC₃N, Astrophys J Supp Series 1978;37:169-194. doi:10.1086/190523.

S. Green, S. Chapman, Astrophys. J. Supp. Series 37, 169-194, doi:10.1086/190523 (1978).