The Structure of a Low-metallicity Giant Molecular Cloud Complex

Articulo

Fecha

2009

Registro en:

http://hdl.handle.net/10533/239559

15010003

WOS:000269244500027

no scielo

eid=2-s2.0-70350608515

https://repositorioslatinoamericanos.uchile.cl/handle/2250/4470898

Institución

ANID (Chile)

Resumen

To understand the impact of low metallicities on giant molecular cloud (GMC) structure, we compare far-infrared dust emission, CO emission, and dynamics in the star-forming complex N83 in the Wing of the Small Magellanic Cloud (SMC). Dust emission (measur

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