LABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud
Context. The amount of molecular gas is a key to understanding the future star formation in a galaxy. Because H2 is difficult to observe directly in dense and cold clouds, tracers such as the CO molecule are used. However, at low metallicities especially,
Detalles Bibliográficos
| Autores: |
Bot, C.,
Rubio, M. |
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| Tipo de recurso: | artículo
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| Estado: | Versión publicada |
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| Fecha de publicación: | 2010 |
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| País: | Chile |
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| Idioma: | inglés |
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| OAI Identifier: | oai:repositorio.anid.cl:10533/240807 |
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| Acceso en línea: | https://hdl.handle.net/10533/240807
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| Access Level: | acceso abierto |
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