Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 106  ·  NGC 4217  ·  NGC 4218  ·  NGC 4220  ·  NGC 4226  ·  NGC 4231  ·  NGC 4232  ·  NGC 4248  ·  NGC 4258  ·  NGC 4346  ·  PGC 166129  ·  PGC 166131  ·  PGC 213956  ·  PGC 213962  ·  PGC 2283887  ·  PGC 2283999  ·  PGC 2284091  ·  PGC 2284225  ·  PGC 2284284  ·  PGC 2284326  ·  PGC 2285022  ·  PGC 2285316  ·  PGC 2285444  ·  PGC 2286144  ·  PGC 2286344  ·  PGC 2286675  ·  PGC 2286698  ·  PGC 2286962  ·  PGC 2286973  ·  PGC 2287164  ·  And 94 more.
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M 106, NGC 4217 galaxy group, Alan Brunelle
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M 106, NGC 4217 galaxy group

Getting plate-solving status, please wait...
M 106, NGC 4217 galaxy group, Alan Brunelle
Powered byPixInsight

M 106, NGC 4217 galaxy group

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Description

Oft imaged grouping of galaxies. Certainly M 106 is the standout, but my favorite is the almost perfectly symmetrical and perfectly edge on NGC 4217. A bit chunky for a spiral, so this galaxy may well be on its way to be a lenticular galaxy, though it is listed as a spiral. Thicker spiral galaxies, at least in the nucleus regions, are supposed to be correlative of the size of the super massive BH at their centers. The bigger the bulge, the bigger the BH. In any case, the perfectness of the edge on of this galaxy attracted the attention of Hubble, for the purpose of studying the distribution of molecular clouds in spiral galaxies. I suggest you take a look at the Hubble photos of this, they are spectacular. I will need a longer fl telescope for that!

My background on this seems to be a bit noisy. I may try to deal with that in a revision. As soon as I have some time.

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Revisions

  • M 106, NGC 4217 galaxy group, Alan Brunelle
    Original
  • M 106, NGC 4217 galaxy group, Alan Brunelle
    B
  • Final
    M 106, NGC 4217 galaxy group, Alan Brunelle
    C

B

Description: Was wanting to correct a strong red cast in the original upload. Oddly, for some reason PI photometric color calibration could not solve this field, even though plate solving and rendering worked great. So I winged it. But given a bit of time to catch up on this, here is what I expect to be the real final version.

Uploaded: ...

C

Description: In being self-critical with some of my recent galaxy images, I have embarked on some revisions. For this one, I have decided that the previous image was probably overly stretched and over contrast enhanced to the extent that M 106's outer disk is rather misrepresented as more dense and detailed than it is relative to the inner region. In doing so, the finer detail within that inner disk was lost to view. My guide was simply my unstretched subs and stack along with other's images. So I am presenting a heavily reprocessed image as the final. For this, I back way out and redid the stacking, taking advantage of doing a false-luminance stack to improve resolution. But in the end, with a more subtle processing hand, I think that my noise reduction also benefitted. This revision does not go as deep as the original, but seeing all the tiny red fuzzies that are there in the original stack kind of misses the point. And I cannot stand the artifacts generated otherwise. There are still a few point-like artifacts in M 106 that were generated with deconvolution, but cannot really be seen unless in full mag view. So don't do that!

In the end, not nearly as dramatic, but then probably more true to M 106. And I much prefer the new 4217 as well as the other smaller galaxies. I believe that I can see more detail in there.

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M 106, NGC 4217 galaxy group, Alan Brunelle