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Paper: Near Infrared Spectroscopy as a Probe of Excitation in Star Formation Regions
Volume: 267, Hot Star Workshop III: the Earliest Stages of Massive Star Birth
Page: 103
Authors: Lumsden, S. L.; Puxley, P. J.; Hoare, M. G.
Abstract: The only bright recombination lines from HII regions in the near-infrared JHK wavebands are due to hydrogen and helium. This paper outlines the potential uses and problems with these lines in setting limits on the form of the emergent ultraviolet stellar radiation field.
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