Abstract
Optical, infrared, and radio observations of He2-10 are presented. Originally classified as a planetary nebula, He2-10 is shown to be a dwarf emission galaxy with a nonthermal radio continuum. Features resembling Wolf-Rayet bands are present in the spectrum. The galaxy is particularly rich in neutral hydrogen and radiates most of its energy in the infrared.
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CITATION STYLE
APA
Allen, D. A., Wright, A. E., & Goss, W. M. (1976). The Dwarf Emission Galaxy He2-10. Monthly Notices of the Royal Astronomical Society, 177(1), 91–97. https://doi.org/10.1093/mnras/177.1.91
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