3D photoionization and kinematical reconstruction of the Planetary Nebula H 2-18

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K. Gesicki; A. A. Zijlstra; M. Hajduk; A. Iwanowska; K. Grzesiak; K. Lisiecki; J Lipinski

doi:10.1017/s1743921323005082

December 1, 2023Proceedings of the International Astronomical Union

3D photoionization and kinematical reconstruction of the Planetary Nebula H 2-18

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Key Points

Photoionization techniques revealed complex kinematics in the planetary nebula H 2-18.
MOCASSIN's 3D models enhance understanding of the spatial density distribution in H 2-18.
HST images were utilized to constrain the nebula's density distribution effectively.
The unique insights from ARGUS 2D spectroscopy contributed to a richer analysis of H 2-18.

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Abstract

The Planetary Nebula H 2-18 is analysed with the full-3D capabilities of the MOCASSIN code. The collected HST images help to constrain the density distribution while the ARGUS 2D spectroscopy provides a new and unique information on kinematics.

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Gesicki et al. (2023) studied this question.

synapsesocial.com/papers/68e5d50830fda0630036afde https://doi.org/10.1017/s1743921323005082

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3D photoionization and kinematical reconstruction of the Planetary Nebula H 2-18

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Abstract

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3D photoionization and kinematical reconstruction of the Planetary Nebula H 2-18

Key Points

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Abstract

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Cite This Study

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