||Spiral Galaxy / M106 / NGC4258 / H43-5
||Canes Venatici (CVN)
||Ra 12h 20m 05s Dec +47° 26’03” (current)
|Size & Distance:
||18.6 x 7.2 Mag 8.3 Apx 24 Million light-years.
|Date & Location:
||04-01-2022 Little Blair Valley, CA
||HaLRGB 120,100,60,60,60.Ha-8x15, L-20x5, RGB 6x10 ea (bin 1x1
||Telescope Engineering Company APO110FL w/ TEC FF @ f/5.74, 631mm, FLI-Atlas focuser.
||Astro-Physics Mach 1 GTOCP4 / ATS 8x36 Pier
||FLI-MLx694 @-25c / FLI CFW1-8 / Guided by SBIG ST-I / w OAG.
||Astrodon 3nm Ha, G2 LRGB
||MaxImDL 6.11, Photoshop CC, CCDStack 2.82, Topaz Studio.
||Sky conditions: Above average seeing, Mid to Low 40’s
Cropped Image Field of view is 55.6 x 49 arcmin. Image Scale 1.48 arcsec/pix
Also in the FOV is NGC4217-4220-4228 being most prominent. Plus many other small galaxies.
Messier 106 (also known as NGC 4258) is a spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781. M106 is at a distance of about 22 to 25 million light-years away from Earth. It is also a Seyfert II galaxy. Due to x-rays and unusual emission linesdetected, it is suspected that part of the galaxy is falling into a supermassive black hole in the center. NGC 4217 is a possible companion galaxy of Messier 106.