Placidus
09-06-2015, 01:37 PM
For us quite exceptional seeing of 1.5 sec arc most of the night.
We've only done the Prawn in H-alpha before, and were most surprised to find that it is rich in SII while weak in OIII. That is most unusual. Given that both OIII and SII emission require the presence of relatively high vacuum, and very hard UV, but SII emission has the added requirement of the presence of material dredged up from deep in a stellar core, it's hard to think of a good explanation.
The good seeing meant that we've captured lots of very fine filigree dust lanes.
Processing was fun: we used our new Asus 8 megapixel monitor which can display 100% of sRGB, and has a viewing angle of 170 deg, so the picture doesn't change as you move your head around. (We haven't figured out how to make it display its native 10 bit colour depth yet).
One can see why it's called the prawn: general shape, two buggy eyes, and even that groove you get down the back when you remove the vein. But it also looks quite convincingly like a yellow sheep going for a swim in a blue billabong. You can see the head toward bottom left, both front legs, the rump and near hind leg, wet matted fur, and a very sheepish expression.
Green: H-alpha 4hrs, Blue: OIII 3hrs, Red: SII 3hrs. Astrodon 3nM. Aspen CG16M at -30C on 20" PlaneWave CDK on MI-750 fork.
Big one (2.5MB) original here. (http://www.mikeberthonjones.smugmug.com/Category/Star-Forming-Regions/i-zx6bkSh/0/O/Prawn%20Nebula%20Ha%204%20OIII%203% 20SII%203hrs.jpg)
We've only done the Prawn in H-alpha before, and were most surprised to find that it is rich in SII while weak in OIII. That is most unusual. Given that both OIII and SII emission require the presence of relatively high vacuum, and very hard UV, but SII emission has the added requirement of the presence of material dredged up from deep in a stellar core, it's hard to think of a good explanation.
The good seeing meant that we've captured lots of very fine filigree dust lanes.
Processing was fun: we used our new Asus 8 megapixel monitor which can display 100% of sRGB, and has a viewing angle of 170 deg, so the picture doesn't change as you move your head around. (We haven't figured out how to make it display its native 10 bit colour depth yet).
One can see why it's called the prawn: general shape, two buggy eyes, and even that groove you get down the back when you remove the vein. But it also looks quite convincingly like a yellow sheep going for a swim in a blue billabong. You can see the head toward bottom left, both front legs, the rump and near hind leg, wet matted fur, and a very sheepish expression.
Green: H-alpha 4hrs, Blue: OIII 3hrs, Red: SII 3hrs. Astrodon 3nM. Aspen CG16M at -30C on 20" PlaneWave CDK on MI-750 fork.
Big one (2.5MB) original here. (http://www.mikeberthonjones.smugmug.com/Category/Star-Forming-Regions/i-zx6bkSh/0/O/Prawn%20Nebula%20Ha%204%20OIII%203% 20SII%203hrs.jpg)