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SN 2023xgo: Helium-rich Type Icn or Carbon-Flash Type Ibn supernova?

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Gangopadhyay, Anjasha, Sollerman, Jesper, Tsalapatas, Konstantinos, Maeda, Keiichi, Dukiya, Naveen, Schulze, Steve, Fransson, Claes, Sarin, Nikhil, Pessi, Priscila J., Singh, Mridweeka, Wise, Jacob, Nakaoka, Tatsuya, Singh, Avinash, Dastidar, Raya, Kawabata, Miho, Qing, Yu-Jing, Das, Kaustav K., Perley, Daniel, Fremling, Christoffer, Taguchi, Kenta, Hinds, K-Ryan, Lunnan, Ragnhild, Teja, Rishabh Singh, Dubey, Monalisa, Ailawadhi, Bhavya, Banerjee, Smaranika, Kawabata, Koji S, Misra, Kuntal, Sahu, Devendra K, Brennan, Sean J., Kasliwal, Mansi M., Ho, Anna Y. C. Q, Bochenek, Aleksandra, Rusholme, Ben, Laher, Russ R., Smith, Roger, Purdum, Josiah, Sravan, Niharika
Format:	Preprint
Publié:	2025
Sujets:	High Energy Astrophysical Phenomena
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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