{"title":"Index","authors":"","doi":"10.1017/9781108553070.024","DOIUrl":"https://doi.org/10.1017/9781108553070.024","url":null,"abstract":"","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"45 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"124750084","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"The Maxwell’s Demon of Star Clusters","authors":"","doi":"10.1017/9781108553070.019","DOIUrl":"https://doi.org/10.1017/9781108553070.019","url":null,"abstract":"","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"15 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"115465055","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Binaries at Very Low Metallicity","authors":"","doi":"10.1017/9781108553070.022","DOIUrl":"https://doi.org/10.1017/9781108553070.022","url":null,"abstract":"","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"126 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"128437207","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Binarity at High Masses","authors":"","doi":"10.1017/9781108553070.012","DOIUrl":"https://doi.org/10.1017/9781108553070.012","url":null,"abstract":"","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"9 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"128334054","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Luminous Blue Variables: Their Formation and Instability in the Context of Binary Interactions","authors":"","doi":"10.1017/9781108553070.013","DOIUrl":"https://doi.org/10.1017/9781108553070.013","url":null,"abstract":"","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"24 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"123009933","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Massive Star Evolution: Binaries as Two Single Stars","authors":"","doi":"10.1017/9781108553070.011","DOIUrl":"https://doi.org/10.1017/9781108553070.011","url":null,"abstract":"","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"4 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"122554087","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Gaia and LSST: Their Importance in Binary Star Research","authors":"G. Beccari, H. Boffin","doi":"10.1017/9781108553070.005","DOIUrl":"https://doi.org/10.1017/9781108553070.005","url":null,"abstract":"","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"1 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2019-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"128532015","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Binary Post-AGB Stars as Tracers of Stellar Evolution","authors":"H. Winckel","doi":"10.1017/9781108553070.009","DOIUrl":"https://doi.org/10.1017/9781108553070.009","url":null,"abstract":"In this chapter the focus is on the properties of post-Asymptotic Giant Branch (post-AGB) stars in binary systems. Their Spectral Energy Distributions (SEDs) are very characteristic: they show a near-infrared excess, indicative of the presence of warm dust, while the central stars are too hot to be in a dust-production evolutionary phase. This allows for an efficient detection of binary post-AGB candidates. It is now well established that the near-infrared excess is produced by the inner rim of a stable dusty disc that surrounds the binary system. These discs are scaled-up versions of protoplanetary discs and form a second generation of stable Keplerian discs. They are likely formed during a binary interaction process when the primary was on ascending the AGB. I will summarise what we have learned from the observational properties of these post-AGB binaries. The impact of the creation, lifetime and evolution of the circumbinary discs on the evolution of the system are yet to be fully understood.","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"3 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2018-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"117087774","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Population Synthesis of Binary Stars","authors":"R. Izzard, Ghina M. Halabi","doi":"10.1017/9781108553070.006","DOIUrl":"https://doi.org/10.1017/9781108553070.006","url":null,"abstract":"Many aspects of the evolution of stars, and in particular the evolution of binary stars, remain beyond our ability to model them in detail. Instead, we rely on observations to guide our often phenomenological models and pin down uncertain model parameters. To do this statistically requires population synthesis. Populations of stars modelled on computers are compared to populations of stars observed with our best telescopes. The closest match between observations and models provides insight into unknown model parameters and hence the underlying astrophysics. In this brief review, we describe the impact that modern big-data surveys will have on population synthesis, the large parameter space problem that is rife for the application of modern data science algorithms, and some examples of how population synthesis is relevant to modern astrophysics.","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"30 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2018-08-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"121374138","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Binaries as Sources of Gravitational Waves","authors":"G. Nelemans","doi":"10.1017/9781108553070.016","DOIUrl":"https://doi.org/10.1017/9781108553070.016","url":null,"abstract":"With the discovery of both binary black hole mergers and a binary neutron star merger the field of Gravitational Wave Astrophysics has really begun. The current advanced LIGO and Virgo detectors are laser interferometers that will improve their sensitivity in the coming years. In the long run, new detectors such as LISA and the Einstein Telescope will have sensitivities that allow the detection of many thousands of sources and ET can observe essentially the whole observable Universe, for heavy black holes. All these measurements will provide new answers to open questions in binary evolution, related to mass transfer, out-of-equilibrium stars and the role of metallicity. In addition, the data will give new constraints on uncertainties in the evolution of (massive) stars, such as stellar winds, the role of rotation and the final collapse to a neutron star or black hole. For black hole binaries, the number of detections is rapidly approaching 10 and the first proper statistical studies of the population can be done soon. In the long run, the thousands of detections by ET will enable us to probe their population in great detail over the history of the Universe. For neutron stars, the first question is whether the first detection GW170817 is a typical source or not. In any case, it has spectacularly shown the promise of complementary electro-magnetic follow-up. For white dwarfs we have to wait for LISA (around 2034) but new detections by e.g. Gaia and LSST will prepare for the astrophysical exploitation of the LISA","PeriodicalId":283497,"journal":{"name":"The Impact of Binary Stars on Stellar Evolution","volume":"553 1","pages":"0"},"PeriodicalIF":0.0,"publicationDate":"2018-07-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"116237750","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}