The [S ii] Spectral Images of the Planetary Nebula NGC 7009. II. Major Axis

Abstract

We derived position–velocity density distribution diagrams along the major (PA = 77°) axis of the elliptical planetary nebula NGC 7009 with the Keck HIRES [S ii ] 6716/6731 Å doublet spectral images. The average densities of the main shell and knots of NGC 7009 derived from the [S ii ] 6716/6731 Å fluxes integrated over the line of sight indicate a density range of N _e = 10 ^3.4 to 10 ^3.9 cm ^−3 , while the local densities from the volume fraction resolved in radial velocities along the line of sight show a considerably large range of about 10 ^2.8 –10 ^4.7 cm ^−3 . The derived projection angle of the major axis of the main shell is ψ ∼ 18.3° (±2°). Assuming that the main shell is an ellipsoidal shell with a ≃ 16″ and b ≃ 6″, we found the range of the expansion velocity, radius, and latitude of four knots and a hot bubble. The four knots at points in symmetrical positions are roughly aligned with the same axis of expansion of latitudes ϕ ∼ ±34.5° (±0.6°): one pair expands at about 35 km s ^−1 close to the main ellipsoidal shell, and the other expands rapidly at about 60 km s ^−1 at a distance of r ∼ 16″. In the latitude range ϕ = 65°–75°, the hot bubble of a relatively large structure expands rapidly with a velocity of 130–150 km s ^−1 . The four knots and hot bubble points, which expand faster than the main shell, appear to have been formed by two to three eruptions at a different epoch from the primary structure formation.

Keywords

• Planetary nebulae
• H II regions
• Interstellar medium
• Post-asymptotic giant branch