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Saturday, July 30, 2011

Info Post





Since my processing technique gets better and the time of year doesn't give any support, I have reprocessed some older images. There is now star colors added and other processing is tweaked too.









IC 410, in Auriga


Ra 05h 22m 39s Dec -33° 31′ 01″








HST-palette, (HST=Hubble Space Telescope)


from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.






Emission nebula IC 410 and an open cluster, NGC1893, inside it are located in constellation Auriga about 12.000 light years from my home town Oulu in Finland. The cloud of glowing gas is over 100 light-years across, sculpted by stellar winds and radiation from embedded open star cluster NGC 1893. 


"Cosmic tadpoles" are potentially sites of ongoing star formation, they are about 10 light-years long. 


Emission from sulfur atoms is shown in red, hydrogen atoms in green, and oxygen in blue hues in this false-color, narrow band composite image above. 







Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.







Original processing can be seen from here:










Processing work flow:


Image acquisition, MaxiDL v5.07.


Stacked and calibrated in CCDStack.


Deconvolution with a CCDSharp, 30 iterations.


Levels, curves and color combine in PS CS3.


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Telescope, Meade LX200 GPS 12" @ f5


Camera, QHY9


Guiding, SXV-AO @ 8Hz


Image Scale, 1,5 arcseconds/pixel

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Exposures:


H-alpha 7x1200s Binned 2x2a


O-III 4x600s, binned 3x3


S-II 3x600s, binned 3x3

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