Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 106  ·  NGC 4248  ·  NGC 4258
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M106 (NGC 4258), Greg Erianne
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M106 (NGC 4258)

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M106 (NGC 4258), Greg Erianne
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M106 (NGC 4258)

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Description

M106 (NGC 4258) is a large intermediate spiral galaxy in the constellation Canes Venatici and is about 22-25 million light-years (ly) from Earth. 

 The dwarf galaxy, NGC 4248 can be seen at the bottom of the image.  In addition, there are numerous galaxies seen surrounding M106 in this image. The edge-on spiral galaxy, NGC  4217 (not shown; 60 million ly away from Earth) is believed to be a companion galaxy to M106.

 One of the things that makes this galaxy very interesting is its active nucleus is classified as a Type 2 Seyfert, which has supermassive black hole at its center and is surrounded by discs of material falling inward toward the black hole.  As the gas consumed by the black hole heats up it emits microwave radiation that gives the galaxy two extra arms visible in light images (not shown in this image) as wisps of gas oriented perpendicularly to the main (star-forming) spiral arms.  There’s a beautiful image of these energetic gas arms here.

 Additionally, M106 contains two supernovae, SN 1981K and SN 2014bc.

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M106 (NGC 4258), Greg Erianne