Sadr region (IC 1318 parts B & C)
The star c Cygni(Sadr, visual magnitude +2.23) is in the center of the cross of the constellation ofCygnus. The surrounding area contains the giant butterfly nebula (IC 1318 parts B & C). It is an emission nebula, but it contains several dark nebulae too, such as basic centerline of powder, separating it in the middle. He took his name because it resembles to a butterfly. It is a highly contrast theme, because of the louminosity in contrast to the surrounding dark nebulae. It is located 5,000 light-years from us, deep in the Orion spiral of our galaxy.
Technical data of the photo:
Takahashi FSQ 106 ED with reducer x 0.73
Ha: 7x30 min bin1
Lum: 7x30 min bin1
Red 5x10 bin2, Green4x10 min bin2, Blue 4x10 min bin2.
Mount AP Mach1 GTO
Camera QSI 683, -20 C
Edit pixinsight, Photoshop
Skyros, July 2014
During my involvement in photographing the "deep sky" I missed the accompaniment of music, as my musical experience guides me. So I decided to fill my astrophotos with my music. From September 2016 as a starting point, therefore, together with the Flaming Star Nebula, I present to You, the ‘Floydish Pulsar I’, as my first musical composition (composition, performance and production by me), always inspired by these images.
Parallel Words ! and Dancing Stars I, complete my first trilogy.
Emjoy !