The Ionization Structure of a Sample of Wind-Driven Nebulae

Details The Ionization Structure of a Sample of Wind-Driven Nebulae The Ionization Structure of a Sample of Wind-Driven Nebulae

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313..483m&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

Scientific paper

We are conducting a study on the energetics and dynamical evolution of the final stages of intermediate and massive stars. Our project includes the study of the ionization structure of the haloes of MSPNe and WRNe, and the detection of a possible shock-heated gas component. We present here the set of observations so far obtained, and preliminary results of the well known PN NGC 6543.

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