Ionization Models for Axi-symmetrical Objects or Jets

Details Ionization Models for Axi-symmetrical Objects or Jets Ionization Models for Axi-symmetrical Objects or Jets

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12...82h&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

Hydrodynamics, Planetary Nebulae: Individual (Ngc 6543, Ngc 6826), Stars: Winds, Outflows

Scientific paper

When we obtain a slit spectrum from nebulous objects, we take a narrow pencil through the image. We must, then, use the model to predict the emission from this pencil beam and compare it with the relevant observations. We present a new scheme for modeling or coupling the photoionization code with 2D hydrodynamic simulation to predict the emission of axi-symmetric photoionized objects or shocked excited objects such as jets or PN halos.

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