NGC 6960 and NGC 6979 Veil Nebula in the Swan

The Veil Nebula is a cloud of Cygnus hot and ionized gas. It is a large, but relatively weak remnant of a supernova. It is estimated that the source supernova exploded around 3,000 B.C. to 6,000 B.C. This Image is the combination of Images obtained with the H-Alpha and LRGB filter. Image Processed in Pixinsight. Data obtained from the Deep Sky West robotic observatory located in Rowe, New Mexico, between June 22, 2016 and August 24, 2016. Team: TelescopeTakahashi FSQ 106 EDX III QSI 683wsg-8 camera Paramount MyT mount Set Astrodon Filters LRGB Tru-Balance E-Series Gen 2 and Astrodom 5nm H-Alpha Filter. Data: H-Alpha: 13x1800 "-20C bin 1x1 Blue: 16x600 "-20C bin 1x1 Green: 16x600 "-20C bin 1x1 Luminance: 16x900 "-20C bin 1x1 Red: 16x600 "-20C bin 1x1 Total integration time: 18.5 hours. If the full screen tab is not enough for you, you can see the image in full resolution by clicking on the Link.