Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1764144 | Advances in Space Research | 2015 | 6 Pages |
Abstract
For analysis of spectrum of a molecule in the interstellar medium, radiative and collisional transition probabilities for rotational transitions in the molecule are required. We have calculated collisional rate coefficients for rotational transitions in ortho and para thioformaldehyde (H2CS), and in ortho and para Silylidene (H2CSi) due to collisions with He atom for kinetic temperatures 10, 20, 30, 40 and 50Â K, following the procedure discussed in our earlier work. The accuracy of collisional rate coefficients may be within a factor of 2.
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Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
M.K. Sharma, Monika Sharma, U.P. Verma, Suresh Chandra,