Celestial hemisphere:  Northern  ·  Constellation: Lacerta (Lac)
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Abell 79, Gary Imm
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Abell 79

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Abell 79, Gary Imm
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Abell 79

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Description

This object is a rarely imaged planetary nebula located 4000 light years away in the constellation of Lacerta at a declination of +55 degrees. The nebula spans 2 arc-minutes in our apparent view, which corresponds to a diameter of just over 2 light years.

The structure of this planetary nebula is unlike any other that I have imaged or seen. I am not going to try to describe the unique shape here when the image does a fine job of showing it. The signal is primarily HII. I am fascinated by the intersecting arcing gas fronts, as well as the tiny lobes which extend inward from the overall oval "loop". The OIII signal is strongest on the inner edge of the loop and shows up in the image as a faint misty cyan shadow, particularly at the bottom inside of the loop.

I was not able to find any explanation of how this unique PN structure was generated. My view is that the surrounding interstellar medium (ISM) is very active and has distorted the typically symmetric shape. Comparing this to the Helix Nebula (NGC 7293) for example, the overall structures look broadly similar (outer HII region with arcing bands and an inner OIII section with lobes that face the center), but the outer features are very distorted in this object.

There is a bright central star but I cannot confirm that this is the source star of the PN.

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