NGC 1512

Autor(i): Alejandro Moreno

Dátum vydania:

NGC 1512 is an SBa-type barred spiral galaxy about 30 million light-years away in the constellation Horologium. The galaxy displays a double ring structure, with a (nuclear) ring around the galactic nucleus and an (inner) further out in the main disk. It also hosts an extended UV disc with at least 200 clusters with recent star formation activity

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