Hostname: page-component-54dcc4c588-sq2k7 Total loading time: 0 Render date: 2025-10-07T15:20:01.652Z Has data issue: false hasContentIssue false
  • English
  • Français

A Multi-Wavelength Analysis of Planetary Nebula NGC 3132 using MUSE, JWST and SPITZER data

Published online by Cambridge University Press:  06 October 2025

Konstantinos Bouvis Open the ORCID record for Konstantinos Bouvis [Opens in a new window]  and
Stavros Akras Open the ORCID record for Stavros Akras [Opens in a new window]
Konstantinos Bouvis*
Affiliation:
Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, National Observatory of Athens, GR 15236 Penteli, Greece
Stavros Akras
Affiliation:
Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, National Observatory of Athens, GR 15236 Penteli, Greece
*
email: konos982@gmail.com
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

MUSE data regarding NGC 3132 were used and analysed through SATELLITE in order to obtain 2D maps of the physico-chemical parameters of the nebula. Furthermore, our results were compared with a 3D photoionisation model built with MOCASSIN with the aim to constrain its parameters. Lastly, we utilized JWST and Spitzer IR data and examined their radial distribution.

Keywords

planetary nebulae: individual (NGC 3132)ISM: moleculesISM: dustextinctionISM: abundancesinfrared: ISM

Information

Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 19 , Symposium S384: Planetary Nebulae: A Universal Toolbox in the Era of Precision Astrophysics , December 2023 , pp. 427 - 428
Check for updates
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2025. Published by Cambridge University Press on behalf of International Astronomical Union

References

Akras, S., Monteiro, H., Walsh, J. R., et al. 2022, MNRAS, 512, 2202. doi: 10.1093/mnras/stac632 CrossRefGoogle Scholar
Akras, S., Gonçalves, D. R., Ramos-Larios, G., et al. 2020, MNRAS, 493, 3800. doi: 10.1093/mnras/staa515 CrossRefGoogle Scholar
Aleman, I. & Gruenwald, R. 2011, AAP, 528, A74. doi: 10.1051/0004-6361/201014978 CrossRefGoogle Scholar
Phillips, J. P., Cuesta, L. C., & Ramos-Larios, G. 2010, MNRAS, 409, 881. doi: 10.1111/j.1365-2966.2010.17372.x CrossRefGoogle Scholar
De Marco, O., Akashi, M., Akras, S., et al. 2022, Nature Astronomy, 6, 1421. doi: 10.1038/s41550-022-01845-2 CrossRefGoogle Scholar
Monreal-Ibero, A. & Walsh, J. R. 2020, AAP, 634, A47. doi: 10.1051/0004-6361/201936845 CrossRefGoogle Scholar
Supplementary material: File

Bouvis and Akras supplementary material

Bouvis and Akras supplementary material
Download Bouvis and Akras supplementary material(File)
File 904 KB