CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy: IV. ALMA observations of organic species at a galactocentric radius of ∼23 kpc
[Context] Single-dish observations suggest that the abundances of organic species in star-forming regions of the outer Galaxy, which are characterised by sub-solar metallicities, are comparable to those found in the local Galaxy.
| Autores: | , , , , , , , , |
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| Tipo de documento: | artigo |
| Estado: | Versão publicada |
| Data de publicação: | 2024 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositório: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/383975 |
| Acesso em linha: | http://hdl.handle.net/10261/383975 https://api.elsevier.com/content/abstract/scopus_id/85209651774 |
| Access Level: | Acceso aberto |
| Palavra-chave: | ISM: molecules Stars: formation |
| Resumo: | [Context] Single-dish observations suggest that the abundances of organic species in star-forming regions of the outer Galaxy, which are characterised by sub-solar metallicities, are comparable to those found in the local Galaxy. |
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