Hyperfine excitation of CN by para- and ortho-H2
Among the interstellar molecules, the CN radical is of particular interest since it is a good probe of cold dark molecular clouds, and especially prestellar cores. Modelling of CN emission spectra from these dense molecular clouds requires the calculation of rate coefficients for excitation by colli...
| Published in: | Monthly Notices of the Royal Astronomical Society Vol. 446. P. L21-L25 |
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| Format: | Article |
| Language: | English |
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| Online Access: | http://vital.lib.tsu.ru/vital/access/manager/Repository/vtls:000525178 Перейти в каталог НБ ТГУ |