Celestial hemisphere:  Northern  ·  Constellation: Ursa Major (UMa)
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Arp 268, Gary Imm
Arp 268, Gary Imm

Arp 268

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Arp 268, Gary Imm
Arp 268, Gary Imm

Arp 268

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Description

This object is a dwarf irregular galaxy located "only" 10 million light-years away in the constellation of Ursa Major. Its apparent diameter is 8 minutes and its actual diameter is 25,000 light years. It has an apparent magnitude of 12 and a low surface brightness of 24.

This object has several identifiers, including Arp 268 and UGC 4305, but its most common name is Holmberg II. Erik Holmberg (1908 – 2000) was a Swedish astronomer who is most famous for his work on the effects of interacting galaxies. The nine low surface brightness galaxies existing in the Holmberg catalog were detected by Holmberg at the Lund Observatory in Sweden. The galaxies were published in three publications from 1950 to 1969.

Because it is so close, we have a peak inside at an unusual amount of galaxy detail, including bubbly pink Ha regions and blue star clusters. Star formation is active in this galaxy. The most interesting thing to me about this image are the giant bubbles of glowing Ha gas, particularly the curving line of bubbles at the top of the galaxy in this image. These bubbles reach sizes up to several thousand light years in diameter. They surround high mass stars which are expelling strong stellar winds. Unlike a spiral or elliptical galaxy, this dwarf galaxy has a weak gravitational field which allows these bubbles to retain their shape.

Several other small galaxies are also visible in the background.

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    Arp 268, Gary Imm
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  • Arp 268, Gary Imm
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Description: Comparison to Original Arp Image

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Arp 268, Gary Imm