Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  PK077+14.1
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Abell 61, Gary Imm
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Abell 61

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Abell 61, Gary Imm
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Abell 61

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Description

This object is a faint planetary nebula located 3000 light years away in the constellation of Cygnus, at a declination of +46 degrees. The nebula is framed by a beautiful star field. Its apparent size to us of 3 arc-minutes corresponds to a true diameter of about 3 light years. The central 17th magnitude variable star (WD1917+461) is plainly visible in the center of the nebula. The OIII signal is much stronger than Ha for this nebula.

The most interesting aspect of this object to me is the faint thin rim around the outside edge of the top half of the nebula. The rim is not present on the lower half. A 1994 paper (The Ionization Structure of Old Planetary Nebulae which Interact with the Interstellar Medium, Tweedy and Kwitter) indicates that this effect is due to interaction with the ISM. Some subtle structure is visible on the inside of the nebula, including what looks like the start of a more transparent region in the central region of the nebula.

Several other PN I have imaged have a similar structure (Strong OIII signal with a rim and a more transparent section in the central region), most notably Abell 39 and Jones 1. However, these other nebulae do not show the same non-symmetric ISM impact as this object.

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