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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https://doi.org/10.1007/978-3-319-57228-4nitial mass. In this introductory chapter, we briefly review the most important aspects concerning the evolution and nucleosynthesis of single stars, form the early stage of its formation to the final stages and death.

rectum

Elementary Probability and Set Theory,y nebulae (CSPN). The most recent observations of cool CSPN progenitors of barium stars, as well as of carbon-rich post-common envelope systems, are providing unique constraints on the mass transfer processes.

rectum

Wave Power and the Djursland Coast,ing a primary close to the current turn-off mass. Rather, their primaries tend to be somewhat more massive and have evolved off the main sequence, filling their Roche lobes in the past, often converting their secondaries into blue straggler stars (but more than 1 Gyr or so ago and thus they are no longer visible today as blue straggler stars).

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Introduction to the Theory of Stellar Evolution,nitial mass. In this introductory chapter, we briefly review the most important aspects concerning the evolution and nucleosynthesis of single stars, form the early stage of its formation to the final stages and death.

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Formation Channels for Blue Straggler Stars,ing a primary close to the current turn-off mass. Rather, their primaries tend to be somewhat more massive and have evolved off the main sequence, filling their Roche lobes in the past, often converting their secondaries into blue straggler stars (but more than 1 Gyr or so ago and thus they are no longer visible today as blue straggler stars).