M-106 and the Canes II Galaxy Group in HaLRGB (David Wood (SDAA TARO))

Celestial hemisphere: Northern · Constellation: Canes Venatici (CVn) · Contains: M 106 · NGC 4217 · NGC 4226 · NGC 4231 · NGC 4232 · NGC 4248 · NGC 4258

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M-106 and the Canes II Galaxy Group in HaLRGB

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M-106 and the Canes II Galaxy Group in HaLRGB

M106 is the largest and the most prominent Canes II galaxy group member. It’s about 24 million light-years away in the Canes Vanatici constellation, located in the Big Dipper area. It is classified as a Seyfert galaxy, most likely having an active galactic nucleus. There is speculation that part of the galaxy is being gobbled up by a supermassive black hole near the center.

The major galaxies in the image are NGC 4258 (M-106), NGC 4217, NGC 4226, NGC 4232, NGC 4231 and NGC 4248.

If you zoom in on the image you'll find a lot of small background galaxies, some looking like streaks of colored light and others with a fair bit of detail.

This image comprises 12 hours of LRGB data and 12 hours of Ha data acquired by TARO in May of 2022.

SDAA AISIG Group

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The “AstroBin Image of the Day and Top Picks”, or IOTD/TP, is a long-running system to promote beautiful, interesting, peculiar, or otherwise amazing astrophotographs, with a focus on technical excellence. Learn more.

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Astrometry.net job	9038204
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M-106 and the Canes II Galaxy Group in HaLRGB

M-106 and the Canes II Galaxy Group in HaLRGB

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Image Index:

Contribution Index (beta):

M-106 and the Canes II Galaxy Group in HaLRGB

M-106 and the Canes II Galaxy Group in HaLRGB

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