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Orbital Period Changes of Recurrent Nova U Scorpii Demonstrate that M$_{\rm ejecta}$=26$\times$M$_{\rm accreted}$ and Is Not a Type Ia Supernova Progenitor

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Bibliographic Details
Main Authors:	Schaefer, Bradley E., Myers, Gordon
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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