![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEgpYvUqyeb3fpm0KmmkhGOcSN_KA1I6t_f3J74db9hEveght4EB24fUBAXD80VfHMCe2tGU7xgz8NjYdU8-zvVUgKv_U_zrv588QDsU4WjuTJditS51YaHyfXbj02DAF6dr3QK_dzDaFtRG/s640/NGC7635+BUBBLE+NEBULA+copycopy.jpg)
60% of the original size
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjVWVFM17fov7upLVDA2-gdPgP2wIhLoSWcwnWvfpDIPIdHCBWKqISdRz-PB5k24FlaB6ObwqNz5WZHeTCDV4dSJUPDpCPpGQk2TJtOoaE5HxKpEgJwAIjs1OAyLWRpDvZ9Lel8u-dOpW-1/s400/NGC7635BUBNEBcopy60%25.jpg)
NGC 7635, also called the Bubble Nebula and Sharpless 162, is a H II region[2] emission nebula in the constellation Cassiopeia. It lies close to the direction of the open cluster Messier 52. The "bubble" is created by the stellar wind from a massive hot, 8.7[2] magnitude young central star, the 15 ± 5 M☉[4] SAO 20575 (BD+60 2522).[7] The nebula is near a giant molecular cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow.[7] It was discovered in 1787 by Friedrich Wilhelm Herschel.[6] The star SAO 20575 or BD+602522 is thought to have a mass of 10-40 Solar masses.
W.O FLT-110 with dedicated field flattener
EQ6 Pro
ST10XME
Astrodon 5nm Ha filter
Baader 8nm SII filter
Baader 8.5nm OIII filter
Ha: 3h 20min
SII: 4h 20min
OIII:4h
Total exposure 11h40min under near full moon from Kallithea Athens Greece.
Anacortes Image of the Day 08/09/2009
1 comment:
Καλά ρε Θοδωρή έγραψες πάλι!!
Αντε και εις ανώτερα!
Ο οδοντίατρός σου...
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