A Detailed Morpho-Kinematic Model of the Eskimo, NGC 2392. A Unifying View with the Cat's Eye and Saturn Planetary Nebulae
Ma. T. Garc\'ia-D\'iaz, J. A. L\'opez, W. Steffen, M. G. Richer

TL;DR
This paper presents a detailed 3D morpho-kinematic model of the Eskimo nebula, revealing its structure and relation to similar planetary nebulae, using high-resolution spectroscopic data and HST imaging.
Contribution
It introduces a comprehensive spatially resolved spectroscopic mapping and a 3D model that unifies the Eskimo nebula with Saturn and Cat's Eye nebulae, considering orientation effects.
Findings
Eskimo nebula is a rotated analog of Saturn and Cat's Eye nebulae.
The model applies broadly to elliptical planetary nebulae with ansae or FLIERS.
The study suggests a common evolutionary sequence for these nebulae.
Abstract
The 3-D and kinematic structure of the Eskimo nebula, NGC 2392, has been notoriously difficult to interpret in detail given its complex morphology, multiple kinematic components and its nearly pole-on orientation along the line of sight. We present a comprehensive, spatially resolved, high resolution, long-slit spectroscopic mapping of the Eskimo planetary nebula. The data consist of 21 spatially resolved, long-slit echelle spectra tightly spaced over the Eskimo and along its bipolar jets. This data set allows us to construct a velocity-resolved [NII] channel map of the nebula with a resolution of 10 km/s that disentangles the different kinematic components of the nebula. The spectroscopic information is combined with HST images to construct a detailed three dimensional morpho-kinematic model of the Eskimo using the code SHAPE. With this model we demonstrate that the Eskimo is a close…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
