Titlebook: Ecology of Blue Straggler Stars; Henri M. J. Boffin,Giovanni Carraro,Giacomo Beccar Book 2015 Springer-Verlag Berlin Heidelberg 2015 Blue

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Blue Stragglers in Globular Clusters: Observations, Statistics and Physics, to point towards a formation channel involving binaries, rather than dynamical encounters. However, the correlation between blue straggler numbers and actual binary numbers—which relies on recently determined empirical binary fractions—is actually . than that with core mass. We explain how this sur

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Blue Stragglers in Clusters and Integrated Spectral Properties of Stellar Populations,ar evolution. Blue straggler stars (BSSs), as discussed intensively in this book both observationally and theoretically, are very important in our context when considering the integrated spectral properties of a cluster, or a simple stellar population. In this chapter, we are going to describe how i

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Book 2015rmation channels; Dynamics of globular clusters; Interpretation of observational data and comparison with models. The book also offers an introductory chapter on stellar evolution written by the editors of the book..

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Dimensions and Properties of Piping,th the observations and the .-body models strongly indicate that the long-period blue-straggler binaries—which dominate the NGC 188 blue-straggler population—are formed by asymptotic-giant (primarily) and red-giant mass transfer onto main-sequence stars. The models suggest that the few non-velocity-

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Best Practices of the CFD Trade,d that multiple channels of BSS formation are likely to take part in producing the observed BSSs, and we point out the strengths and weaknesses of each the formation channel in respect to the observational constraints. Finally we point out directions to further explore the origin of BSS, and highlig

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Applied Computational Materials Modeling there are more possible configurations which produce blue stragglers, and there are differing contributions to the blended light of the system. The effects of rotation may be substantial in both collision and merger products, and could result in significant mixing unless angular momentum is lost sh

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https://doi.org/10.1007/978-3-319-30866-1 to point towards a formation channel involving binaries, rather than dynamical encounters. However, the correlation between blue straggler numbers and actual binary numbers—which relies on recently determined empirical binary fractions—is actually . than that with core mass. We explain how this sur