Evolution of Close Binary Systems

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Supernova Type Ia progenitors from merging double white dwarfs - Using a new population synthesis model (2012, methodology): “Therefore we evaluated this track by performing detailed numerical calculations using thev binary stellar-evolution code originally developed by Eggleton (Eggleton 1971, 1972; Yakut & Eggleton 2005, and references therein) and updated as described in Pols et al. (1995) and Glebbeek et al. (2008).”
V1309 Scorpii: merger of a contact binary (2010, background): “If the outer Roche lobes (dimensions can be calcu- lated from Yakut & Eggleton 2005) are assumed to be filled by the components, the luminosity increases by∼35%, while the distance becomes 3.5± 0.7 kpc.”