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JWST Observations of SN 2024ggi I: Interpretation and Model Comparison of the Type II Supernova 2024ggi at 55 days Past Explosion

Fuente: arXiv
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Bibliographic Details
Main Authors: Baron, E., Ashall, C., DerKacy, J. M., Hoeflich, P., Medler, K., Shahbandeh, M., Fereidouni, E., Pfeffer, C. M., Mera, T., Hoogendam, W. B., Shiber, S., Auchettl, K., Brown, P. J., Burns, C. R., Burrow, A., Coulter, D. . A., Engesser, M., Folatelli, G., Fox, O., Galbany, L., Guolo, M., Hinkle, J. T., Huber, Mark E., Hsiao, E. Y., de Jaeger, T., Jones, D. O., Kumar, S., Lu, J., Mazzali, P. A., Morrell, N., Phillips, M. M., Rest, A., Suntzeff, N. B., Shappee, B. J., Shi, Jennifer, Stritzinger, M. D., Strolger, L., Temim, T., Tinyanont, S., Tucker, M., Wang, L., Wang, Q., Yang, Y.
Format: Preprint
Published: 2025
Subjects:
Solar and Stellar Astrophysics
High Energy Astrophysical Phenomena
Online Access:
Acceder al recurso
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