Publication | Open Access
Submillimeter line emission from LMC N159W: a dense, clumpy PDR in a low metallicity environment
34
Citations
60
References
2008
Year
Microwave SpectroscopyGalaxy FormationPhotometryEngineeringPhysicsCosmic PlasmaNatural SciencesSpectroscopyStellar StructureClumpy PdrAstrophysical PlasmaSubmillimeter Line EmissionLmc N159wLarge Magellanic CloudSynchrotron RadiationHigh-energy AstrophysicsLow MetallicityAstrophysics
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.
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