EnriqueAstro
M27_Final_V2
This is the HOO version of M27 using the Narrow-band Normalization script from Bill Blanshan.
Imaging telescope :
Askar Apochromatic 80/600 mm Askar 80PHQ
Imaging camera
ZWO Optical ASI533MC (CMOS)
Mount:
Equatorial iOptron GEM-45
Guiding telescope:
Orion Refractor 60/240 mm
Guiding camera:
ZW0 ASI120MM mini (CMOS)
Filters
Optolong Multi-Narrowband L-Ultimate 2.00"
Lights: 150 x 300 sec
Total lights integration time: 12:30 hours
M27 (Dumbbell, NGC6853m Apple Core) is a planetary Nebula residing at about 1,200 light-years from Earth, discovered by Charles Messier in 1764. It contains dense nodes of gas at its core, the glowing gas around the central star (a White Dwarf) is formed by ionized hydrogen (Orange-red) and ionized oxygen (Blue) and is a consequence of the star shedding its outer layers. M27 is the brightest planetary nebula in the night sky.
M27_Final_V2
This is the HOO version of M27 using the Narrow-band Normalization script from Bill Blanshan.
Imaging telescope :
Askar Apochromatic 80/600 mm Askar 80PHQ
Imaging camera
ZWO Optical ASI533MC (CMOS)
Mount:
Equatorial iOptron GEM-45
Guiding telescope:
Orion Refractor 60/240 mm
Guiding camera:
ZW0 ASI120MM mini (CMOS)
Filters
Optolong Multi-Narrowband L-Ultimate 2.00"
Lights: 150 x 300 sec
Total lights integration time: 12:30 hours
M27 (Dumbbell, NGC6853m Apple Core) is a planetary Nebula residing at about 1,200 light-years from Earth, discovered by Charles Messier in 1764. It contains dense nodes of gas at its core, the glowing gas around the central star (a White Dwarf) is formed by ionized hydrogen (Orange-red) and ionized oxygen (Blue) and is a consequence of the star shedding its outer layers. M27 is the brightest planetary nebula in the night sky.