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HD 32188
HD 32188 is suspected variable star in the northern constellation of Auriga. It is a shell star, which means it has a peculiar spectrum indicating there is a circumstellar disk of gas around the star's equator. While the spectrum matches a luminosity class of III, the derived class is type I; suggesting this is actually a supergiant star.〔
==References==
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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