Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...456..591m&link_type=abstract
Astronomy and Astrophysics, Volume 456, Issue 2, September III 2006, pp.591-597
Astronomy and Astrophysics
Astrophysics
4
Planetary Nebulae: Individual: Ic 5217, Ism: Jets And Outflows
Scientific paper
Aims.Identification of the structural components and analysis of the internal kinematics in the planetary nebula IC 5217. Methods: .Narrow-band images and high resolution long-slit spectra in the Hα, [N ii] and [O iii] emission lines, and VLA 6 cm continuum data. Results: .IC 5217 is composed of a very bright equatorial ring, open bipolar lobes, off-axis point-symmetric features, on-axis distant faint regions, and an off-axis very elongated bipolar structure. The ring, open lobes, point-symmetric features and distant faint regions appear as elements of a single point-symmetric bipolar shell with a very narrow waist. This shell presents an axis ratio of ~37 and an aspect ratio of ~5. The 6 cm data show that the ring is an extremely flat disk with a central hole. Expansion velocity in the ring ranges from ≤10 km s-1 in He ii up to ≃27 km s-1 in [N ii], whereas a velocity of ~460 km s-1 is estimated for the polar regions of the bipolar shell. Strong acceleration of the outer regions of the ring is observed. The elongated bipolar structure probably represents a highly collimated (aspect ratio ~12), high velocity cylindrical-like shell. A collimated agent (wind or jet) would account for the shaping of the bipolar shell if this agent has operated in the direction perpendicular to the equatorial disk. The point-symmetric features and cylindrical shell are probably related to collimated ejections but that occurred when the basic nebular shape had already been established.
Ayala Sandra
Guillén P. F.
Miranda Luis F.
Vazquez Ruben
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