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- Data collection using:
CCD Commander
CCDSoft
FocusMax
PinPoint
TheSky6 Pro
- Image Calibration - Maxim DL
- Image Registration - Maxim DL
- Image Stacking - Maxim DL
- Post processing in Adobe Photoshop CS4 Extended
The central star is a binary with a period of ~68d varying by nearly 1 magnitude. The central object is a highly reddened B5 dwarf that is 1700 pc (5600 ly) distant. It is thought that PK36-1.1 contains 3 pairs of bipolar lobes shown in this drawing from the linked reference from 3 separate episodes, all younger than 10,000 years.
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