Publication Abstracts
Green and Chapman 1978
, and S. Chapman, 1978: Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC3N. Astrophys. J. Supp. Ser., 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.
- Get PDF (1.9 MB. Document is scanned; no OCR)
- PDF documents require the free Adobe Reader or compatible viewing software to be viewed.
- Go to journal article webpage
Export citation: [ BibTeX ] [ RIS ]
BibTeX Citation
@article{gr02700w, author={Green, S. and Chapman, S.}, title={Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC3N}, year={1978}, journal={Astrophysical Journal Supplement Series}, volume={37}, pages={169--194}, doi={10.1086/190523}, }
[ Close ]
RIS Citation
TY - JOUR ID - gr02700w AU - Green, S. AU - Chapman, S. PY - 1978 TI - Collisional excitation of interstellar molecules: Linear molecules CO, CS, OCS, and HC3N JA - Astrophys. J. Supp. Ser. JO - Astrophysical Journal Supplement Series VL - 37 SP - 169 EP - 194 DO - 10.1086/190523 ER -
[ Close ]