Search for an interstellar Si2C molecule: A theoretical prediction
| dc.contributor.author | Chandra, Suresh | |
| dc.date.accessioned | 2012-03-09T04:46:49Z | |
| dc.date.available | 2012-03-09T04:46:49Z | |
| dc.date.issued | 2011-07-06 | |
| dc.description.abstract | We suggest that Si2C molecule may be identi¯ed in astronomical objects through its transitions 414 ! 505, 515 ! 606, 212 ! 303, 313 ! 404, and 111 ! 202 at 15.9, 5.1, 33.6, 24.9, and 42.3 GHz in absorption even against the cosmic 2.7 K background, in a region having low temperature. The absorption phenomenon is found rather large in the ¯rst two transitions. Dependence of results on the set of molecular parameters is discussed. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/967 | |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | IUCAA Preprints;11/04 | |
| dc.subject | Interstellar molecules | en_US |
| dc.subject | Si2C | en_US |
| dc.title | Search for an interstellar Si2C molecule: A theoretical prediction | en_US |
| dc.type | Article | en_US |
| dc.type | Book | en_US |