Barnard's Galaxy... NGC 6822 in HaLRGB, Steve Timmons

Barnard's Galaxy... NGC 6822 in HaLRGB

Barnard's Galaxy... NGC 6822 in HaLRGB, Steve Timmons

Barnard's Galaxy... NGC 6822 in HaLRGB

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Description

NGC 6822, commonly known as Barnard's Galaxy, is a member of the Local Group and lies approximately 1.6 million light-years away in the constellation Sagittarius. Star formation is actively taking place in many vast areas of ionized hydrogen gas, known as HII regions; these regions can be likened to miniature versions of Orion’s Great Nebula. When massive, young stars form within these clouds of gas and dust, their intense ultraviolet radiation ionizes the surrounding hydrogen, causing it to emit a characteristic red glow. In NGC 6822, the HII regions are notably vibrant and numerous, showcasing a bustling environment of stellar birth. NGC 6822, however, is not classified as a starburst galaxy. While it does contain several active star-forming regions, its rate of star formation is not as intense as that observed in galaxies categorized as starburst galaxies. Starburst galaxies are characterized by an exceptionally high rate of star formation, leading to rapid consumption of their interstellar gas. In contrast, NGC 6822, an irregular dwarf galaxy, exhibits a more moderate and sustained star-forming activity.

This image is a collaborative effort between my friend Don Waid and myself.

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Barnard's Galaxy... NGC 6822 in HaLRGB, Steve Timmons