P. Puxley
Gemini 8m Telescopes Project, 950 N. Cherry Ave., Tucson AZ 85719
New observations of hydrogen recombination lines in the compact HII region K3-50a are presented. They cover a broad wavelength range from the near-IR (Br and others, observed with ISO), through sub-mm and mm transitions (H26 - H30 from JCMT and H40 - H68 from Nobeyama) to radio wavelengths. The line fluxes are compared with a simple model.
Appears in the proceedings of "Star Formation with ISO", Lisbon, 1997.
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