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Morpho-kinematic Properties of Wolf–Rayet Planetary Nebulae

  • Authors: A. Danehkar

A. Danehkar 2022 The Astrophysical Journal Supplement Series 260 .

  • Provider: AAS Journals

Caption: Figure 5.

3D mesh models of PNs M 3-30, Hb 4, IC 1297, Th 2-A (Danehkar 2015), Pe 1-1, M 1-32, M 3-15, M 1-25, Hen 2-142, K 2-16, MGC 6578, M 2-42 (Danehkar et al. 2016), NGC 6567, and NGC 6629, (a) before and (b) after rendering at the best-fitting inclinations and orientations. In each mesh model, there is a main shell (blue color) and other parts, like point-symmetric knots (red color) and collimated outflows and thin halos (gray color). The 3D mesh models (14 models in the X3D file format) are available in the interactive figure online.

(An interactive version of this figure is available.)

An interactive version of this figure is available in the online journal.

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