Morpho-kinematic modelling of gaseous nebulae with Shape

Details Morpho-kinematic modelling of gaseous nebulae with Shape Morpho-kinematic modelling of gaseous nebulae with Shape

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005rmxac..23...19s&link_type=abstract

The Ninth Texas-Mexico Conference on Astrophysics (Eds. S. Torres-Peimbert & G. MacAlpine) Revista Mexicana de Astronomía y Astr

Astronomy and Astrophysics

Astrophysics

Planetary Nebulae: Individual (Ngc6369), Stars: Mass Loss

Scientific paper

We present a powerful new tool to disentangle the 3-D geometry and kinematic structure of gaseous nebulae. The method consists of combining commercially available digital animation software to simulate the 3-D structure and expansion pattern of the nebula with a dedicated, purpose built rendering software that produces the final images and long slit spectra which are compared to the real data. In this contribution we show results for the complex planetary nebula NGC369 based on long slit spectra obtained at the San Pedro Mártir observatory.

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