Articulo
LABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud
Fecha
2010Registro en:
15010003
WOS:000284625300012
no scielo
eid=2-s2.0-78649370523
Institución
Resumen
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,