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Figure 22. M57, the Ring Nebula in Lyra, enlarged and cropped from the image in Figure
21. Note the fine structure detail in the upper right portion of the ring and the wisps of
nebulosity visible inside the ring around the central star. The fact that the above image can
bear this degree of enlargement and still show this amount of detail is amazing and is
largely due to the sub-pixel accuracy of the autoguiding used to acquire the data.
With this initial success, the author felt he could confidently move on to long exposure imaging
with a cooled CCD camera and purchased the SBIG STL 11000M shown in Figures 19A and
19B, which is one of SBIG‟s self-guiding cameras. The results, some of which are shown in
Figures 23 and 24, show dramatic improvements over those obtained with the DSLR.
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