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http://nopr.niscpr.res.in/handle/123456789/25193Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Sharma, Arvind K | - |
| dc.contributor.author | Chandra, Suresh | - |
| dc.date.accessioned | 2013-12-30T05:44:25Z | - |
| dc.date.available | 2013-12-30T05:44:25Z | - |
| dc.date.issued | 2001-12 | - |
| dc.identifier.issn | 0975-1041 (Online); 0019-5596 (Print) | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/25193 | - |
| dc.description | 765-767 | en_US |
| dc.description.abstract | Laboratory detection of NaSH molecule in absorption has been reported by Kagi & Kawaguchi, Astrophys J , 491 (1997) L129. They observed only a-type rotational transitions of the molecule. The reason for not observing b-type rotational transitions was assigned to a small value of b-component of electric dipole moment (μb = 0.63 D) as compared to a-component of electric dipole moment (μa = 8.91 D) of the molecule. The b-type transitions may be detected in emission in interstellar medium having low densities. However, it is not feasible to detect b-type rotational transitions in the absorption spectrum. | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | NISCAIR-CSIR, India | en_US |
| dc.rights |  CC Attribution-Noncommercial-No Derivative Works 2.5 India | en_US |
| dc.source | IJPAP Vol.39(12) [December 2001] | en_US |
| dc.title | Detection of rotational lines of NaSH molecule | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJPAP Vol.39(12) [December 2001] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJPAP 39(12) 765-767.pdf | 479.36 kB | Adobe PDF | View/Open |
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