3-D Modeling of the collimated outflows of M1-32 and M 2-42

Details 3-D Modeling of the collimated outflows of M1-32 and M 2-42 3-D Modeling of the collimated outflows of M1-32 and M 2-42

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012hell.conf...27a&link_type=abstract

10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011. Edited by Io

Astronomy and Astrophysics

Astronomy

Scientific paper

We present high resolution long-slit spectra from San Pedro Martir catalogue (Lopez et al. in prep.) of M1-32 & M2-42 planetary nebulae and their modeled PV diagrams using the 3D morpho-kinematic code SHAPE. We find high-speed collimated outflows, surrounded by a thick dusty torus/ring. The same SHAPE model is able to fit both planetary nebulae assuming one cylindrical velocity field for the outflows and one Hubble-law for the dusty torus/ring concluding that they may be akin objects which just appear at different projections.

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