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Ecology of Blue Straggler Stars
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Ecology of Blue Straggler Stars
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The existence of blue straggler stars (BSS), which appear younger, hotter, and more massive than their siblings, is at odds with a simple picture of stellar evolution, as such stars should have exhausted their nuclear fuel and evolved long ago to become cooling white dwarfs. As such, BSS could just be some quirks but in fact their understanding requires a deep knowledge of many different areas in astronomy, from stellar evolution through cluster dynamics, from chemical abundances to stellar populations. In November 2012, a workshop on this important topic took place at the ESO Chilean headquarters in Santiago. The many topics covered at this workshop were introduced by very comprehensive invited reviews, providing a unique and insightful view on the field. These reviews have now become chapters of the first ever book on BSS.
Forward citations
Cited by 1 Pith paper
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Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations
N-body models of NGC 3532 produce only 0-8 stellar mergers, too few to explain the cluster's ~37% blue main-sequence population, disfavoring the merger origin for its slow rotators.
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