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Star-Forming Region S106

Hubble Space Telescope's high resolution combines with the Subaru Telescope's wide field-of-view to reveal a depiction of star-forming region S106 that is not possible from either telescope alone. The bipolar S106 shows bright gas in two distinct lobes. The faint stars located near the nebulosity are brown dwarf candidates associated with the region of star formation.



This composite image combines optical and near-infrared astronomical data from the Hubble Space Telescope with mid-infrared data from the ground-based Subaru Telescope, located on Mauna Kea in Hawaii.


Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and the Subaru Telescope (National Astronomical Observatory of Japan)

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