| dc.contributor.author | Yan, M. | |
| dc.contributor.author | Dalgarno, A. | |
| dc.contributor.author | Klemperer, W. | |
| dc.contributor.author | Miller, A. E. S. | |
| dc.date.accessioned | 2019-09-27T13:18:36Z | |
| dc.date.issued | 2000 | |
| dc.identifier.citation | Yan, M., A. Dalgarno, W. Klemperer, and A. E. S. Miller. 2000. “The CO Cameron Band Emission in the Red Rectangle.” Monthly Notices of the Royal Astronomical Society 313 (2): L17–18. https://doi.org/10.1046/j.1365-8711.2000.03421.x. | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | http://nrs.harvard.edu/urn-3:HUL.InstRepos:41417378 | * |
| dc.description.abstract | The origin of the strong CO Cameron band emission in the Red Rectangle is investigated. From a comparison of laboratory spectroscopic data and astronomical observations in combination with chemical modelling, it is concluded that the Cameron band emission of CO originates from the dissociative recombination of HCO+, and its intensity provides a measure of the product of the density of HCO+ ions and the electron density, integrated along the line of sight. | |
| dc.language.iso | en_US | |
| dc.publisher | Oxford University Press | |
| dash.license | LAA | |
| dc.title | The CO Cameron band emission in the Red Rectangle | |
| dc.type | Journal Article | |
| dc.description.version | Version of Record | |
| dc.relation.journal | Monthly Notices of the Royal Astronomical Society | |
| dash.depositing.author | Dalgarno, Alexander::501fae4cfad8b04754ee2838c45fc5d0::600 | |
| dc.date.available | 2019-09-27T13:18:36Z | |
| dash.workflow.comments | 1Science Serial ID 65923 | |
| dc.identifier.doi | 10.1046/j.1365-8711.2000.03421.x | |
| dash.source.volume | 313;2 | |
| dash.source.page | L17-L18 | |
