Test of planetary nebula evolution models by distance-independent parameters

Details Test of planetary nebula evolution models by distance-independent parameters Test of planetary nebula evolution models by distance-independent parameters

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aca....43..359k&link_type=abstract

Acta Astronomica, vol. 43, no. 4, p. 359-370

Astronomy and Astrophysics

Astronomy

2

Hertzsprung-Russell Diagram, Planetary Nebulae, Stellar Evolution, Dynamic Models, Photoionization, Stellar Mass

Scientific paper

The difficulty in comparing observations with theoretical evolutionary tracks in the Herztsprung-Russell diagram is reviewed. A number of distance-independent paramenters are suggested as alternative means to test evolutionary models of planetary nebulae. The need for a ionization-dynamical model to provide proper interpretation of observed physical parameters is emphasized. The procedure on how an integrated model of planetary nebula evolution can be constructed is outlined.

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