Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  MQ J131214.42+364901.0  ·  MQ J131223.19+363648.0  ·  MQ J131224.06+364249.8  ·  MQ J131243.53+363418.8  ·  MQ J131251.57+364836.4  ·  MQ J131257.33+363849.3  ·  MQ J131258.28+363423.5  ·  MQ J131320.68+363134.9  ·  MQ J131321.88+363034.0  ·  MQ J131323.86+363820.8  ·  MQ J131326.99+365318.5  ·  MQ J131329.32+363513.2  ·  MQ J131333.37+364644.9  ·  MQ J131335.26+363356.9  ·  MQ J131335.96+363913.4  ·  MQ J131347.32+363157.0  ·  MQ J131348.93+365334.0  ·  MQ J131358.26+364805.6  ·  MQ J131409.92+362508.2  ·  MQ J131414.17+362807.8  ·  MQ J131416.28+364330.6  ·  MQ J131430.43+364724.2  ·  NGC 5033  ·  PGC 166160  ·  PGC 2079742  ·  PGC 2080543  ·  PGC 2083200  ·  PGC 2086098  ·  PGC 2086185  ·  PGC 2086293  ·  And 66 more.
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NGC5033 a large Seyfert galaxy, John Favalessa
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NGC5033 a large Seyfert galaxy

Getting plate-solving status, please wait...
NGC5033 a large Seyfert galaxy, John Favalessa
Powered byPixInsight

NGC5033 a large Seyfert galaxy

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Description

After all the cloudy nights in February, March, April, May and June, I woke up to the fact that I mostly missed galaxy season 😩!  I had hopes of going deep on many galaxies and clusters this year.  Only got a few nights of a few galaxies and one cluster…oh, well there’s always next year.  

One that I did get was NGC5033.  I’m surprised that is not often imaged here on astrobin, but I found it an interesting target from my backyard in April.   At 60MLYs it’s in the wheelhouse for my 9.25HD.   Certainly, an interesting galaxy.  It’s huge, like twice the size of our Milky Way.  We are not looking face on.  So the spiral arm at the top seems to extend above the plane.  And then there’s a blob at 1 o’clock.  It's pretty cool at full resolution...I might do a mouse over.  Some research revealed that this is one of the nearest large Seyfert galaxies.   Lots of eye candy in the frame also...what the hey is PGC45927?  

From Wikipedia: any of a class of galaxies known to have active nuclei.  Such galaxies were named for the American astronomer Carl K. Seyfert, who first called attention to them in 1944.  They have quasar-like nuclei (very luminous sources of electromagnetic radiation that are outside of our own galaxy) with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, their host galaxies are clearly detectable. Seyfert galaxies account for about 10% of all galaxies and are some of the most intensely studied objects in astronomy, as they are thought to be powered by the same phenomena that occur in quasars, although they are closer and less luminous than quasars. These galaxies have supermassive black holes at their centers which are surrounded by accretion discs of in-falling material.

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