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Contains:  NGC 4395
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NGC 4395 Spiral Galaxy, 



    
        

            Jerry Macon
NGC 4395 Spiral Galaxy
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NGC 4395 Spiral Galaxy

Technical card


Dates:Feb. 2, 2019

Frames:Astrodon Gen 2 RGB 36mm: 104x200" (gain: 99.00) -20C bin 1x1

Integration: 5.8 hours

Avg. Moon age: 27.41 days

Avg. Moon phase: 5.01%

Bortle Dark-Sky Scale: 4.00

Temperature: -5.00


Basic astrometry details

Astrometry.net job: 3223888

RA center: 12h 25' 49"

DEC center: +33° 33' 0"

Pixel scale: 0.501 arcsec/pixel

Orientation: 357.674 degrees

Field radius: 0.293 degrees


Resolution: 3315x2610

Locations: Dark Star Observatory, Taos, New Mexico, United States

Data source: Own remote observatory

Remote source: Non-commercial independent facility

Description

Images from the following two scopes (piggybacked) contributed to this image:
AG12+ASI1600MM at .70 asec/pix (RGB)
TV127is+ASI183MM at .75 asec/pix. (RGB)
They were all registered to the best R image taken on the AG12.
L is derived from the combined RGB.
Imaged on nights of Feb/2/2019 and Feb/8/2019.

NGC 4395 is a low surface brightness spiral galaxy with a halo that is about 8′ in diameter. It has several wide areas of greater brightness running northwest to southeast. The one furthest southeast is the brightest. Three of the patches have their own NGC numbers: 4401, 4400, and 4399 running east to west. The nucleus of NGC 4395 is active and the galaxy is classified as a Seyfert. It is notable for containing one of the smallest supermassive black hole with an accurately-determined mass. The central black hole has a mass of "only" 300,000 Sun masses, which would make it a so-called "intermediate-mass black hole".
(Wikipedia)

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Author

jmacon
Jerry Macon
License: Attribution Creative Commons
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NGC 4395 Spiral Galaxy, 



    
        

            Jerry Macon