Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.281l..57m&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Vol. Vol. 281, No. 3, p. L57 - L61
Astronomy and Astrophysics
Astronomy
15
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.
Bryce Myfanwy
Clayton C. A.
Meaburn John
Walsh Jonathan R.
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