The global motions of the cometary knots in the Helix planetary nebula (NGC 7293).

Astronomy and Astrophysics – Astronomy

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Planetary Nebulae: Individual: Ngc 7293, Planetary Nebulae: Radial Velocities, Planetary Nebulae: Kinematics, Planetary Nebulae: Structure

Scientific paper

Systematic measurements of the radial velocities of a significant sample of the Helix cometary knots have been made in a sustained period of exceptionally good "seeing". This kinematical information has been combined with [O III] 5007-Å images of the whole of the Helix nebula to identify the location of each knot. A global expansion velocity of ≍10 km s-1 for the system of knots has been found, which is far less than the 24 km s-1 general expansion of the Helix nebula. A model is favoured in which the cometary knots are relics of condensations in the precursor, red giant/AGB, slow, dense wind now overrun by faster shells (and perhaps fast winds) generated after the formation of the planetary nebula.

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