Phantoms Of The Northern Sky

Returning after a summer break, my first target this autumn has been a fascinating and challenging deep-sky imaging object SH2-185, located in the constellation of Cassiopeia. Often referred to as the Gamma Cassiopeiae Nebula, it is closely associated with the very bright star Gamma Cassiopeiae (γ Cas), which dominates the surrounding star field. SH2-185 encompases the wider HII region that also includes two distinct nebulae IC59 and IC63, which together create the familiar appearance of the Ghost of Cassiopeia. The entire SH2-185 complex (see below) is therefore a combination of both emission and reflection nebulae (see details in the annotated image below).

Although the two components are usually treated as a single imaging target, IC 59 and IC 63 have different appearances and physical relationships with Gamma Cassiopeiae. The differences explain both the colours and challenges involved in processing the data. IC 59 lies to the north and north-east of Gamma Cassiopeiae, where its appearance is dominated by the reflected starlight. IC 63, the Ghost Nebula, lies south-west of the main star and is generally the more conspicuous of the two with its curved, comet-like shape and bright ionisation front which make it especially distinct. The adjacent Gamma Cassiopeiae is a hot, massive, rapidly rotating B-type star. Its intense ultraviolet radiation interacts with the surrounding gas and dust, thereby highlighting the area and especially the aforesaid structures within IC 59 and IC 63.

 

SH2-185 has been a rewarding but demanding target because of the bright main star and faint surrounding nebulosity which present very different imaging and processing challenges. In this case I chose to process the data in two ways, each of which highlight different qualities: SHO (top of the page) and HOS (above). The results reveal a complex and dynamic region of the northern sky within our galaxy; the importance of Ha in shaping the final image can be seen in the image below.

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