Analysis of hydrogen cyanide hyperfine spectral components towards star forming cores
Although hydrogen cyanide has become quite a common molecular tracing species for a variety of astrophysical sources, it, however, exhibits dramatic non-LTE behaviour in its hyperfine line structure. Individual hyperfine components can be strongly boosted
| Authors: | ; ; ; ; |
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| Format: | Article |
| Status: | Published version |
| Publication date: | 2011 |
| Country: | Chile |
| Institution: | Agencia Nacional de Investigación y Desarrollo |
| Repository: | Articulos_ANID |
| Language: | English |
| OAI Identifier: | oai:repositorio.anid.cl:10533/241061 |
| Online Access: | https://hdl.handle.net/10533/241061 |
| Access Level: | Open access |
| Summary: | Although hydrogen cyanide has become quite a common molecular tracing species for a variety of astrophysical sources, it, however, exhibits dramatic non-LTE behaviour in its hyperfine line structure. Individual hyperfine components can be strongly boosted |
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