| 书目名称 | Observational and Theoretical Studies on Dwarf-nova Outbursts |
| 编辑 | Mariko Kimura |
| 视频video | |
| 概述 | Nominated as an outstanding Ph.D. thesis by Kyoto University, Japan.Explores the physical mechanisms of new types of outbursts in dwarf novae through optical observations and numerical simulations.Int |
| 丛书名称 | Springer Theses |
| 图书封面 |  |
| 描述 | .Accretion disks are ubiquitous in our universe, and produce intense brightening.How does the gas in the disk lose its angular momentum to release massive amounts of gravitational energy? This is one of the biggest open questions in astronomy. This book studies four types of newly detected outbursts in dwarf novae through optical observations and/or numerical simulations and puts forward physical interpretations of these outbursts on the basis of the disk instability model, the most plausible model for dwarf-nova outbursts. It demonstrates that the disk-instability model can explain rich variety in dwarf-nova outbursts if some new aspects are taken into account (e.g. the extremely slow growth of tidal instability and thermal instability in the disk misaligned against the binary orbital plane). Moreover, it shares valuable insights on the evolution of binary systems by finding period bouncers and dwarf novae with F-type companion stars, which are rare objects.. |
| 出版日期 | Book 2020 |
| 关键词 | Accretion Disks; White Dwarfs; Cataclysmic Variables; Binary-Star Evolution; Optical Observations; Disk I |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-981-15-8912-6 |
| isbn_softcover | 978-981-15-8914-0 |
| isbn_ebook | 978-981-15-8912-6Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor |
发表于 2025-3-21 18:40:13
