M33
Triangulum Galaxy

10.1” f/4.5   Mallincam DS432cTEC with 0.5 focal reducer
Exposures = 15-25 sec, Live-stacked frames = 20-25 (45 total), Gain = 15 of 250 

The size of M33 here as seen from the city via EAA techniques appears to be about 25′ across, with the brighter portion appearing in the SW or bottom-half of the disk. Various light and dark concentrations, dust clouds, and HII regions throughout the loose spiral arm structure can be seen. One such region is NGC 604, appearing as a slightly blurred bright star at about 10 o’clock from the core. M33 is thought to be a satellite of M31 and is approximately the same distance (slightly further) away.

North is at 11 o’clock, East at 8 o’clock