  We have made subarcsecond-resolution images of the central 10" of the
Wolf-Rayet dwarf galaxy He 2-10 at 11.7 microns, using the Long Wavelength
Spectrometer on the Keck Telescope. The spatial distribution of the infrared
emission roughly agrees with that of the rising spectrum radio sources seen by
Kobulnicky & Johnson (1999) and confirms that those sources are compact HII
regions rather than SNR or other objects. The infrared sources are more
extended than the subarcsecond rising spectrum radio sources, although the
entire complex is still less than 5" in extent. On sizescales of 1" the
infrared and radio emission are in excellent agreement, with each source
requiring several hundred to a thousand O stars for excitation. The nebulae lie
in a flattened disk-like distribution about 240 by 100 pc and provide all of
the flux measured by IRAS for the entire galaxy in the 12 micron band; 30% of
the total IRAS flux from the galaxy emanates from one 15-30 pc source. In this
galaxy, intense star formation, probably triggered by an accretion event, is
confined to a central disk which breaks up into distinct nebulae which
presumably mark the sites of young super star clusters.
