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Light-curve analysis of the classical nova YZ Ret: revisit with fully self-consistent nova outburst models
Izumi Hachisu, Mariko Kato
YZ Ret is a well observed nova from the first detection of an X-ray flash phase in classical novae until the end of a supersoft X-ray source phase. We have reanalyzed multiwaveleng…
Identification of a superbright nova in our Galaxy: revisiting the light curve analyses of the candidate novae CP Lac, CP Pup, V838 Her, V597 Pup, V5583 Sgr, and V5589 Sgr
Izumi Hachisu, Mariko Kato
The two very fast novae in our Galaxy, V1500 Cyg and V1674 Her, reached the absolute magnitude of . These brightest novae are identified as superbri…
A multiwavelength light curve analysis of the very fast nova V1723 Sco
Izumi Hachisu, Mariko Kato
We have analyzed multiwavelength light curves of the very fast nova V1723 Sco, based on our fully self-consistent nova explosion models. The time-stretching method gives the distan…
Upper bound of ejecta mass in a nova outburst
Izumi Hachisu, Mariko Kato
We present the maximum ejecta mass and the maximum ratio of ejecta mass and accreted mass of a nova for various white…