  We present sub-arcsecond resolution millimeter-wave images of a circumstellar
disk in the Bok globule CB26. The presence of an edge-on disk is confirmed by
the dust continuum morphology and the velocity field of 13CO emission, which
displays a Keplerian rotation pattern about an axis perpendicular to the long
axis of the dust emission. We deduce a mass ~0.3 Msun for the obscured central
star. The disk is optically thick at mm wavelengths inside 120 AU, has a
symmetric 20 degree warp beyond 120 AU, an outer radius of ~200 AU, and a mass
of at least 0.1 Msun. We suggest that the CB26 system is in an intermediate
stage between deeply embedded protostellar accretion disks and the more
evolved, perhaps protoplanetary, disks around T Tauri stars.
