A Dynamical Model for PNe with WR-Type Central Stars

Details A Dynamical Model for PNe with WR-Type Central Stars A Dynamical Model for PNe with WR-Type Central Stars

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15...78m&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Ism: Kinematics And Dynamics, Planetary Nebulae: General, Stars: Agb And Post-Agb

Scientific paper

In this work we present the preliminary results of a dynamical analysis
on a homogeneously observed sample consisting of 21 planetary nebulae
with central stars of the [WC] type (WRPNe) from the list of Tylenda,
Acker, & Stendholm (1993).

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