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Izumi Hachisu

University of Tokyo

287

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The UBV Color Evolution of Classical Novae. IV. Time-stretched (U − B)0–(M B − 2.5 log f s) and (V − I)0–(M I − 2.5 log f s) Color–Magnitude Diagrams of Novae in Outbursts

2021 Astrophysical Journal Supplement Series
- Izumi Hachisu
- Mariko Kato
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The $UBV$ Color Evolution of Classical Novae. IV. Time-Stretched $(U-B)_0$-$(M_B-2.5\log f_{\rm s})$ and $(V-I)_0$-$(M_I-2.5\log f_{\rm s})$ Color-Magnitude Diagrams of Novae in Outburst

2020 arXiv: Solar and Stellar Astrophysics
- Izumi Hachisu
- Mariko Kato
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Supersoft X-ray phases of recurrent novae as an indicator of their white dwarf masses

2020 Publications of the Astronomical Society of Japan
- Mariko Kato
- Izumi Hachisu
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A Theory for the Maximum Magnitude versus Rate of Decline Relation of Classical Novae

2020 The Astrophysical Journal
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Supersoft X-Ray Phases of Recurrent Novae as an Indicator of their White Dwarf Masses

2020 arXiv: Solar and Stellar Astrophysics
- Mariko Kato
- Izumi Hachisu
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A Theory for the Maximum Magnitude versus Rate of Decline Relation of Classical Novae

2020 The Astrophysical Journal
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ASASSN-16oh: A Nova Outburst with No Mass Ejection—A New Type of Supersoft X-Ray Source in Old Populations

2020 The Astrophysical Journal
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Supersoft X-ray phases of recurrent novae as an indicator of their white dwarf masses

2020 Publications of the Astronomical Society of Japan
- Mariko Kato
- Izumi Hachisu
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A Theory for the Maximum Magnitude versus Rate of Decline (MMRD) Relation of Classical Novae

2020 arXiv: Solar and Stellar Astrophysics
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ASASSN-16oh: nova outburst with no-mass-ejection -- A new type of supersoft X-ray sources in old populations

2020 arXiv: Solar and Stellar Astrophysics
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