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What determines the $γ$-ray luminosities of classical novae?

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Craig, Peter, Aydi, Elias, Chomiuk, Laura, Stone, Ashley, Strader, Jay, Chong, Atticus, Li, Kwan-Lok, Fan, Jhih-Ling, Bahramian, Arash, Buckley, David A. H., Izzo, Luca, Kawash, Adam, Metzger, Brian D., Mukai, Koji, Linford, Justin D., Orio, Marina, Sokoloski, J. L., Sokolovsky, Kirill V., Tremou, Evangelia, Walter, Frederick M., Fló, Joan Guarro, Boussin, Christophe, Charbonne, Stéphane, Garde, Olivier, Belyakov, Konstantin, Monard, Libert A. G., Hambsch, Franz-Josef, Thomas, Neil
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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