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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Dimensions and Properties of Piping,te of knowledge about FBSSs, drawn from an extensive literature that I searched with the aid of the ., and .. The search prior to 2000 is spotty and I make no claim of completeness. In documenting various topics I tried to use references that acknowledge important earlier investigations..Extensive .

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https://doi.org/10.1007/978-1-4615-0531-0GCs). The BSS specific frequency, radial distribution, chemical composition and rotational properties are presented and discussed in the framework of using this stellar population as probe of GC internal dynamics. In particular, the shape of the BSS radial distribution has been found to be a powerfu

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Carlos H. Rojas-Fernandez BSc(Pharm), PharmDions overfills its Roche lobe. In this Chapter, we overview the theoretical understanding of mass transfer via Roche lobe overflow: classification, how both the donor and of the accretor respond to the mass transfer on different timescales (adiabatic response, equilibrium response, superadiabatic re

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Wave Power and the Djursland Coast,d via mass transfer within a binary. We review how computer simulations show that stellar collisions are likely to lead to relatively little mass loss and are thus effective in producing a young population of more-massive stars. The number of blue straggler stars produced by collisions will tend to

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Best Practices of the CFD Trade,their observational predictions. These include mass transfer during binary stellar evolution—case A/B/C and D (wind Roche-lobe overflow) mass transfer, stellar collisions during single and binary encounters in dense stellar cluster, and coupled dynamical and stellar evolution of triple systems. We a

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Applied Computational Materials Modelingongoing mass transfer have all been studied in some detail. The products of stellar collisions retain memory of their parent stars and are not fully mixed. Very high initial rotation rates must be reduced by an unknown process to allow the stars to collapse to the main sequence. The more massive col

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https://doi.org/10.1007/978-3-319-30866-1ch on topics also discussed elsewhere in this book, such as the discovery and implications of bimodal radial distributions and the “double sequences” of blue stragglers that have recently been found in some clusters. However, we will focus particularly on the search for a “smoking gun” correlation b