Titlebook: Observational and Theoretical Studies on Dwarf-nova Outbursts; Mariko Kimura Book 2020 The Editor(s) (if applicable) and The Author(s), un

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Mariko Kimurahistory. If by now we are fairly confident most of these events occurred the way we imagine they occurred, we owe it to a rich suite of cosmological observations, whose precision is ever-increasing. On the other hand, there remain several open questions which near-future cosmological observations mi

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General Introduction, aim of this dissertation. Dwarf novae are one subclass of cataclysmic variables composed of a white dwarf and a low-mass star. An accretion disk is formed around the white dwarf by the transferred gas from the low-mass star. The most characteristic observational feature of dwarf novae is intermitte

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Conclusions, posed in Chap.?1. The conclusion is that the disk-instability model has potential for explaining all kinds of outbursts in dwarf novae if new aspects are taken into account, since this research succeeded to present physically feasible explanations to at least four kinds of newly discovered light va