NICMOS Peers Through Dust to Reveal Young Steller Disks. A View of DG Tau B
Depicts: DG Tau B
Copyright: D. Padgett (IPAC/Caltech), W. Brandner (IPAC), K. Stapelfeldt (JPL) and NASA
Show in archive: true
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.
Last Update: 1 September 2019