265 citations · 1k across the 20 of their papers we have counts for
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Rotational mixing in tidally locked massive main-sequence binaries
S. E. de Mink, M. Cantiello, N. Langer +1
One of the main uncertainties in evolutionary calculations of massive stars is the efficiency of internal mixing. It changes the chemical profile inside the star and can therefore…
Modelling the evolution and nucleosynthesis of carbon-enhanced metal-poor stars
O. R. Pols, R. G. Izzard, M. Lugaro +1
We present the results of binary population simulations of carbon-enhanced metal-poor (CEMP) stars. We show that nitrogen and fluorine are useful tracers of the origin of CEMP star…
Evolution of stellar collision products in open clusters. II. A grid of low-mass collisions
E. Glebbeek, O. R. Pols
In a companion paper we studied the detailed evolution of stellar collision products that occurred in an -body simulation of the old open cluster M67 and compared our detailed m…
Evolution of stellar collision products in open clusters. I. Blue stragglers in N-body models of M67
E. Glebbeek, O. R. Pols, J. R. Hurley
Stellar collisions are an important formation channel for blue straggler stars in globular and old open clusters. Hydrodynamical simulations have shown that the remnants of such co…
Rotational mixing in close binaries
S. E. de Mink, M. Cantiello, N. Langer +5
Rotational mixing is a very important but uncertain process in the evolution of massive stars. We propose to use close binaries to test its efficiency. Based on rotating single ste…
Fluorine in carbon-enhanced metal-poor stars: a binary scenario
M. Lugaro, S. E. de Mink, R. G. Izzard +8
A super-solar fluorine abundance was observed in the carbon-enhanced metal-poor (CEMP) star HE 1305+0132 ([F/Fe] = +2.90, [Fe/H] = -2.5). We propose that this observation can be ex…