Rotational excitation of NS+ by H2 revisited: A new global potential energy surface and rate coefficients
Due to the lack of specific collisional data, the abundance of NS+ in cold dense interstellar clouds was determined using collisional rate coefficients of CS as a substitute. To better understand the chemistry of sulfur in the interstellar medium, further abundance modeling using the actual NS+ coll...
| Published in: | Journal of chemical physics Vol. 156, № 20. P. 204311-1-204311-7 |
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| Main Author: | |
| Other Authors: | , |
| Format: | Article |
| Language: | English |
| Subjects: | |
| Online Access: | http://vital.lib.tsu.ru/vital/access/manager/Repository/koha:001001275 |