Low-ionization pairs of knots in planetary nebulae: physical properties and excitation

Details Low-ionization pairs of knots in planetary nebulae: physical properties and excitation Low-ionization pairs of knots in planetary nebulae: physical properties and excitation

2009-06-22

arxiv.org/abs/0906.4134v2

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

The paper contains 11 pages (6 figures and 5 tables). Accepted for publication in MNRAS; added last paragraph for subsection 7

Scientific paper

We obtained optical long-slit spectra of four planetary nebulae (PNe) with low-ionization pair of knots, namely He 1-1, IC 2149, KjPn 8 and NGC 7662. These data allow us to derive the physical parameters and excitation of the pairs of knots, and those of higher ionization inner components of the nebulae, separately. Our results are as follows. 1) The electron temperatures of the knots are within the range 9500 to 14500 K, similar to the temperatures of the higher ionization rims/shells. 2) Typical knots' densities are 500 to 2000 cm^{-3}. 3) Empirical densities of the inner rims/shells are higher than those of the pairs of knots, by up to a factor of 10. Theoretical predictions, at variance with the empirical results, suggest that knots should be denser than the inner regions, by at least a factor of 10. 4) Empirical and theoretical density contrasts can be reconciled if we assume that at least 90% of the knots' gas is neutral (likely composed of dust and molecules). 5) By using Raga et al. (2008) shock modeling and diagnostic diagrams appropriated for spatially resolved PNe, we suggest that high-velocity shocked knots traveling in the photoionized outer regions of PNe can explain the emission of the pairs of knots analysed in this paper.

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