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T Tauri lies on an arc of reflection nebulosity which extends approximately 3$^{\prime\prime}$ N and 2$^{\prime\prime}$ SW from the star. This nebula has a characteristic width of 0.5$^{\prime\prime}$, is concave open toward the nearby Burnham's Nebula, and is closely aligned with the optical polarization vector of the system. The morphology T Tau's edge-brightened cometary nebula is similar to models of scattered light from a flared, optically thick disk observed from 45 degrees above the equator plane. No optical counterpart to the infrared companion is seen to a limiting magnitude of V= 23.
WFPC2 images of HL Tauri show that this object is entirely reflection nebulosity at optical wavelengths. No stellar source is visible to a limiting magnitude of V$=$ 26, a result which dictates a significant upward revision of the luminosity and mass estimates for HL Tau. The V-I color of the nebula is dominated by foreground extinction, with only small internal color changes. The bright core of the nebula has an east-west elongation of 1$^{\prime\prime}$ and has an unusual morphology. We will discuss the implications of these results for i). HL Tau's stellar type and ii). models for the distribution of the circumstellar matter.
