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  • The JWST/MIRI view of the planetary nebula NGC 6302 I.: a UV irradiated torus and a hot bubble triggering PAH formation
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The JWST/MIRI view of the planetary nebula NGC 6302 I.: a UV irradiated torus and a hot bubble triggering PAH formation

Fuente: arXiv
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Bibliographic Details
Main Authors: Matsuura, Mikako, Volk, Kevin, Kavanagh, Patrick, Balick, Bruce, Wesson, Roger, Zijlstra, Albert A., Dinerstein, Harriet L., Peeters, Els, Sterling, N. C., Cami, Jan, Barlow, M. J., Kastner, Joel, Walsh, Jeremy R., Waters, L. B. F. M., Hirano, Naomi, Aleman, Isabel, Bernard-Salas, Jeronimo, Bhatt, Charmi, Blommaert, Joris, Clark, Nicholas, Jones, Olivia, Justtanont, Kay, Kemper, F., Kraemer, Kathleen E., Lagadec, Eric, Laming, J. Martin, Molster, F. J., Baez, Paula Moraga, Monteiro, H., Richards, Anita M S, Sahai, Raghvendra, Sloan, G. C., Torki, Maryam, van Hoof, Peter A. M., Wright, Nicholas J., Wilson, Finnbar, Csukai, Alexander
Format: Preprint
Published: 2025
Subjects:
Solar and Stellar Astrophysics
Astrophysics of Galaxies
Online Access:
Acceder al recurso
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Internet

https://arxiv.org/abs/2508.19332

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