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,
Detalhes bibliográficos
| Autores: |
Bot, C.,
Rubio, M. |
|---|
| Formato: | artículo
|
|---|
| Estado: | Versión publicada |
|---|
| Fecha de publicación: | 2010 |
|---|
| País: | Chile |
|---|
| Idioma: | inglés |
|---|
| OAI Identifier: | oai:repositorio.anid.cl:10533/240807 |
|---|
| Acesso em linha: | https://hdl.handle.net/10533/240807
|
|---|
| Access Level: | acceso abierto |
|---|
