Articulo
Submillimeter line emission from LMC N159W: a dense, clumpy PDR in a low metallicity environment
Astronomy & Astrophysics
Registro en:
15010003
15010003
Autor
Pineda, J. L.
Bronfman, L.
May, J.
Rubio, M.
Institución
Resumen
Context. Star formation at earlier cosmological times took place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation in such an environment. Aims. The physical and chemical state of th FONDAP FONDAP