V392 Persei: A Γ-Ray Bright Nova Eruption from a Known Dwarf Nova
F. J. Murphy-Glaysher,M. J. Darnley,E. J. Harvey,A. M. Newsam,K. L. Page,S. Starrfield,R. M. Wagner,C. E. Woodward,D. M. Terndrup,S. Kafka,T. Arranz Heras,P. Berardi, E. Bertrand, R. Biernikowicz,C. Boussin,D. Boyd,Y. Buchet, M. Bundas,D. Coulter, D. Dejean,A. Diepvens,S. Dvorak,J. Edlin,T. Eenmae, H. Eggenstein, R. Fournier,O. Garde, J. Gout, D. Janzen, P. Jordanov,H. Kiiskinen, D. Lane, R. Larochelle,R. Leadbeater, D. Mankel, G. Martineau,I Miller, R. Modic,J. Montier,M. Morales Aimar, E. Muyllaert,R. Naves Nogues, D. O'Keeffe,A. Oksanen,M. Pyatnytskyy, R. Rast, B. Rodgers,D. Rodriguez Perez, F. Schorr, E. Schwendeman,S. Shadick, S. Sharpe,F. Soldan Alfaro, T. Sove,G. Stone,T. Tordai, R. Venne,W. Vollmann,M. Vrastak,K. Wenzel Monthly Notices of the Royal Astronomical Society（2022）
Key words
accretion,accretion discs,stars: individual (V392 Per),novae,cataclysmic variables,X-rays: stars,transients: novae
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