The Jet from the Black Hole in the M87 Galaxy!

M87 Galaxy Showing Jet from Black Hole at its center. 14×240 sec, Gain 11, Offset 31, QHY183c cooled to -13C, UHC-S filter, Televue TV-85 at F/5.6, SharpCap 3.2.

I’ve tried this before with little success, but this time the jet of M87 shows quite well in this nearly 1 hour exposure.  The amount of energy to shoot out a jet this long is enormous!

M87 Galaxy Showing Jet from Black Hole at its center. 14×240 sec, Gain 11, Offset 31, QHY183c cooled to -13C, UHC-S filter, Televue TV-85 at F/5.6, SharpCap 3.2.  Detail Crop.

It even shows the characteristic blue color of the synchrotron radiation of electrons spiraling in a magnetic field.

Supernova in M61! Another M13 Globular Shot, Too.

Supernova SN2020jfo in M61. 248×30 sec, Gain 30, Offset 31, Bin 2, QHY183c at -10C, UHC-S filter, Televue TV-85 at F/5.6. Detail Crop.
Supernova SN2020jfo in M61. 248×30 sec, Gain 30, Offset 31, Bin 2, QHY183c at -10C, UHC-S filter, Televue TV-85 at F/5.6.  Full field view.

 

I imaged the galaxy above and the globular below on Sunday, May 10, 2020.  Very nice weather that day and a pretty good evening, too.   Being I had to work the next day, I cut the session short and only got data on two objects.

 

M13 Globula Cluster. 100×30 sec, Gain 42 and 1hr (60×60 sec) at Gain 30, Offset 31, QHY183c at -10C, UHC-S filter, Televue TV-85 at F/5.6.

Imaging Session April 30, 2020

M63, the Sunflower Galaxy. 121×60 sec @ Gain 30, Offset 15, QHY183c at -10C, UHC-S filter, Televue TV-85 at F/5.6
M5 Globular Cluster.. 172×60 sec @ Gain 30, Offset 15, QHY183c at -10C, UHC-S filter, Televue TV-85 at F/5.6
M27 Planetary Nebula. 60×60 sec @ Gain 30, Offset 15, QHY183c at -10C, UHC-S filter, Televue TV-85 at F/5.6

The Sunflower Galaxy was the second time this year for imaging it, so I combined the two data sets and got this detail view below.  It is 3.77 hrs total time:

M63, the Sunflower Galaxy. 152×30 sec, Gain 42, 121×60 sec @ Gain 30, Offset 15, QHY183c at -10C, UHC-S filter, Televue TV-85 at F/5.6.