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JWST/MIRI detects the dusty SN1993J about 30 years after explosion

Fuente: arXiv

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Bibliographic Details
Main Authors:	Szalai, Tamás, Zsíros, Szanna, Jencson, Jacob, Fox, Ori D., Shahbandeh, Melissa, Sarangi, Arkaprabha, Temim, Tea, De Looze, Ilse, Smith, Nathan, Filippenko, Alexei V., Van Dyk, Schuyler D., Andrews, Jennifer, Ashall, Chris, Clayton, Geoffrey C., Dessart, Luc, Dulude, Michael, Dwek, Eli, Gomez, Sebastian, Johansson, Joel, Milisavljevic, Dan, Pierel, Justin, Rest, Armin, Tinyanont, Samaporn, Brink, Thomas G., De, Kishalay, Engesser, Michael, Foley, Ryan J., Gezari, Suvi, Kasliwal, Mansi, Lau, Ryan, Marston, Anthony, O'Steen, Richard, Siebert, Matthew, Skrutskie, Michael, Strolger, Lou, Wang, Qinan, Williams, Brian J., Williams, Robert, Xiao, Lin, Zheng, WeiKang
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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