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 lines detected, 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.
Captured in bad seeing, a test of the Equipment.
Luminace: 1 x 300s (Total: 5min) Bin:2x2
Red: 1 x 300s (Total: 5min) Bin:2x2
Green: 1 x 300s (Total: 5min) Bin:2x2
Blue: 1 x 300s (Total: 5min) Bin:2x2
ASA N12 Astrograph F/3.6
3" Wynne Reducer Corrector 0.73x
Atik 490 EX camera @-20C
Valla Observatory (FROSON, Sweden)
March 14, 2015
Images calibrated and processed in AstroPix
Calibration by applying Flat-Field
Only luminace channel used
Scale: 0.92 arcsec/pix
FOW: 52x42 arcmin