Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 106  ·  NGC 4248  ·  NGC 4258
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Spiral Galaxy M106, Steven Bellavia
Spiral Galaxy M106
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Spiral Galaxy M106

Getting plate-solving status, please wait...
Spiral Galaxy M106, Steven Bellavia
Spiral Galaxy M106
Powered byPixInsight

Spiral Galaxy M106

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Description

Galaxy M106, NGC 4258 , is an intermediate spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781. M106 is at a distance of about 23.5 million light-years away from Earth. M106 contains an active nucleus classified as a Type 2 Seyfert, and a central supermassive black hole. A companion galaxy, NGC 4248, is to the lower right.

The addition of Hydrogen Alpha data faintly reveals some star-forming regions as well as the galactic jets caused by matter ejected from the super massive black hole and slamming into other material, heating it up violently.  

Revision B is a screenshot comparing the broadband light (left) to the narrowband H-alpha data (right), which hides some regions while revealing others, including jets and star-forming regions:

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Revisions

  • Final
    Spiral Galaxy M106, Steven Bellavia
    Original
  • Spiral Galaxy M106, Steven Bellavia
    B

B

Description: Comparison of broadband (left) and narrowband H-alpha (right), which hides some regions while revealing others, such as the jets streaming from the core of the galaxy.

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Spiral Galaxy M106, Steven Bellavia

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