Object  Ngc 6357
Info

Ngc 6357 AKA as the Crab. This image is looking at the heart of the object and its true shape is not defined. Ngc 6357 is located in the constellation Scorpius, a large star forming region, having an apparent size of about 50 arc minutes (about 400 light years). At its centre is the open star cluster Pismis 24, birthing extremely bright and blue stars. The overall nebula contains some of the most massive stars ever discovered.
The overall red glow to the inner star forming region results from the emission of ionized hydrogen gas.
The surrounding nebula has a complex network of gas, dark dust and residing within this are newly forming and already formed stars. The myriad of detailed patterns are the effect of interactions between interstellar winds, radiation pressures, magnetic fields, and gravity. NGC 6357 is a very faint emission nebula, needing a large aperture telescope or long exposure photography to reveal the faint structures. It lies about 8,000  L.yrs. away

Date Ha- 13/ 5/ 08 Lum-31/ 5/ 08 and GB data 31/ 6/ 08
Location BayTop Observatory- Streaky Bay South Australia
Instrument Home built 10" Newtonian (Bob Royce primary) and an Antares 1/20th wave secondary with MPCC coma corrector. System working @ native f4/ 1016 FL  1.35 arcsec/pixel- FOV  23.3x29.4
Mount Celestron CI700 controlled by a Mel Bartels Goto Control System with Vexta PK264m-01b motors with a pulley and belt system
Camera (CCD) Starlight Xpress HX916 monochrome CCD with Atik manual filter wheel.
Exposures Ha:164 L: 80Ha(R):32G:32B:32' [4' sub exposures all unbinned and Sigma combined] No dark frames removed.
Guiding Orion 80ED refractor F7.5 with a Starlight Xpress HX516 CCD. Mounted via a side by side accessory plate.                    
Filters Astronomik typeII clr  RGB filter set
Notes/ Conditions

 Conditions- Taking the Ha seeing was a little average but the transparency was good. Similar conditions taking the lum. The night when taking the colour, I decided due to the deteriorating conditions to only capture green and blue channels and use the Ha data as a sub for the the red channel. Wind and dust produced more than normal bloating to the G & B channels. Still very dry for winter here.