  We present an infrared imaging study of the low-mass pre-main sequence binary
system Haro 6-10. This system is one of a handful in which the
optically-visible primary has the characteristics of a normal T Tauri star,
while the secondary is a so-called "infrared companion" (IRC), a strongly
extincted object which emits most of its luminosity in the infrared. A speckle
holographic technique was used to produce nearly diffraction-limited images on
three nights over a one-year period starting in late 1997. The images show that
the IRC is obscured and surrounded by a compact, irregular, and variable
nebula. This structure is in striking contrast to the well-ordered edge-on disk
associated with HK Tauri B, the extincted companion to another T Tauri star of
similar age. A new, resolved intensity peak was found 0".4 southwest of the
IRC. We suggest that it may represent light scattered by a clump of dusty
material illuminated by starlight escaping along an outflow-carved cavity in
the IRC envelope. The primary star became fainter and the companion became more
extended during the observing period.
