An excellent example of the complementary nature of Hubble's instruments may be found by comparing the infrared NICMOS image of DG Tau B to the visible-light Wide Field and Planetary Camera 2 (WFPC2) image of the same object. WFPC2 highlights the jet emerging from the system, while NICMOS penetrates some of the dust near the star to more clearly outline the 50 billion-mile-long dust lane (the horizontal dark band, which indicates the presence of a large disk forming around the infant star). The young star itself appears as the bright red spot at the corner of the V-shaped nebula.
Object Name: DG Tau B
Image Type: Astronomical/Annotated
Credit (left): D. Padgett (IPAC/Caltech), W. Brandner (IPAC), K. Stapelfeldt (JPL)
Credit (right): Chris Burrows (STScI)
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