Krishna Swamy, K. S. ; A'hearn, M. F. (2000) On so in comets Earth, Moon, and Planets, 84 (2). pp. 109-113. ISSN 0167-9295
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Official URL: http://www.springerlink.com/content/g66q8655uxg5m8...
Related URL: http://dx.doi.org/10.1023/A:1026717925132
Abstract
The solution of the statistical equilibrium equations for the SO molecule is used to estimate the expected intensities of microwave lines. The observed fluxes of the microwave lines of SO in Comet Hale-Bopp require approximately 1.8 × 1028 mol/sec which give fluxes in the A3Π - X3Σ-bands below the observable limit, consistent with the observations.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Springer-Verlag. |
| Keywords: | Comet Hale-bopp; Molecules; SO and SO2 |
| ID Code: | 18309 |
| Deposited On: | 17 Nov 2010 12:48 |
| Last Modified: | 04 Jun 2011 09:40 |
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