description Sh2-225 Overview
Sh2-225 is an emission nebula and H II region in the constellation Auriga. It lies in the Milky Way's Perseus Arm and is catalogued in the Sharpless list of H II regions. The region is associated with ionized hydrogen and an embedded infrared source, making it a subject of observations of massive-star formation; one proposed ionizing star is the O-type star LSV+4046. Because it is faint and compact in optical images, it is primarily of interest to astronomers and astrophotographers.
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