M106 & Friends

Continuing the galaxy season theme, I returned to image Messier 106 last month, one of the brightest galaxies in the northern sky. Located about 24 million light-years from Earth in the constellation Canes Venatici, it is similar in size and luminosity to the much closer Andromeda Galaxy (2.5 million light-years), which therefore appears much larger.  Classified as an active Seyfert galaxy, M106’s core contains a supermassive black and thereby, energetic activity produces unusual arms made of hot glowing gas, which is only visible in radio and X-ray wavelengths.

 

The region around M106 is also very rich with other galaxies, I counted at least another seven. One close companion is NGC 4248, a smaller irregular galaxy gravitationally linked to M106. Nearby in the same field is NGC 4217, an edge-on spiral galaxy appearing thin and elongated through telescopes. More distant background galaxies such as NGC 4220, NGC 4231, and NGC 4232 can also be seen in deep astrophotography images, giving the area a crowded and dramatic appearance.

It’s been six years since my first and only image of M106, which can be see here.  At the time I was thrilled to capture this exciting galaxy but this time the Bortle-4 sky of Somerset has unveiled much more detail and colour than before; it’s always good to see progress with my imaging. Notwithstanding, it was something of a shock that after pre-processing the data using PixInsight’s WBPP calibration and stacking software, the High Rejection from the luminance revealed numerous satellites that had passed overhead, which does not bode well for astronomers in the future!