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JWST Spectroscopy of SN Ia 2022aaiq and 2024gy: Evidence for Enhanced Central Stable Ni Abundance and a Deflagration-to-Detonation Transition

Fuente: arXiv

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Bibliographic Details
Main Authors:	Kwok, Lindsey A., Liu, Chang, Jha, Saurabh W., Blondin, Stéphane, Larison, Conor, Miller, Adam A., Dai, Mi, Foley, Ryan J., Filippenko, Alexei V., Andrews, Jennifer E., Andrews, Moira, Auchettl, Katie, Badenes, Carles, Brink, Thomas G., Davis, Kyle W., Flörs, Andreas, Galbany, Lluís, Graur, Or, Howell, D. Andrew, Kumar, Sahana, Könyves-Tóth, Réka, LeBaron, Natalie, Macrie, Colin W., Maeda, Keiichi, Maguire, Kate, McCully, Curtis, Meza-Retamal, Nicolas E., Gonzalez, Estefania Padilla, Pakmor, Rüdiger, Pearson, Jeniveve, Piro, Anthony L., Polin, Abigail, Rehemtulla, Nabeel, Rojas-Bravo, César, Sand, David J., Sangkachan, Chita, Schwab, Michaela, Sears, Huei, Singh, Mridweeka, Subrayan, Bhagya M., Taggart, Kirsty, Temim, Tea, Terwel, Jacco H., Tinyanont, Samaporn, Vinkó, József, Wang, Xiaofeng, Wheeler, J. Craig, Yang, Yi, Zheng, WeiKang
Format:	Preprint
Published:	2025
Subjects:	High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2510.09760