Cosmic pillars of cold molecular gas and clouds of dark dust lie within Sharpless 171, a star-forming region some 3,000 light-years away in the royal constellation Cepheus. This tantalizing false-color skyscape spans about 20 light-years across the nebula's bright central region. It also highlights the pervasive glow of emission from atomic gas using narrowband filters and a color palette made popular in Hubble Space Telescope images. Powering the nebular glow are the young, hot stars of a newly formed cluster, Berkeley 59. Of course, this star-forming region is entry number 171 in the famous 1959 catalog of emission nebulae compiled by astronomer Stewart Sharpless.
explanation from : NASA apod 2008 October
Tricolor Emission Line Image
Instruments and exposure data:
W.O FLT110 with dedicated TMB field flattener
FeatherTouch 3'' focuser
Starizona MicroTouch autofocuser
W.O ZS80 ED
SBIG ST10XME CFW9
Meade DSI
Filters:
SII 8nm Baader Planetarium
Ha 5nm Astrodon
OIII 8.5nm Baader Planetarium
Sky-Watcher EQ6 Pro
SII :30*15min bin1x1
Ha :30*15min bin1x1
OIII:30*15min bin1x1
Total exposure time:22h30min
SII :30*15min bin1x1
Ha :30*15min bin1x1
OIII:30*15min bin1x1
Total exposure time:22h30min
1 comment:
Amazing!!!!!!!!!!
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