Selma E. de Mink
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Binary interaction dominates the evolution of massive stars
H Sana, SE De Mink, A de Koter, N Langer, CJ Evans, M Gieles, E Gosset, ...
Science 337 (6093), 444-446, 2012
Rotating massive main-sequence stars-I. Grids of evolutionary models and isochrones
I Brott, SE de Mink, M Cantiello, N Langer, A de Koter, CJ Evans, I Hunter, ...
Astronomy & Astrophysics 530, A115, 2011
Massive binaries as the source of abundance anomalies in globular clusters
SE De Mink, OR Pols, N Langer, RG Izzard
Astronomy & Astrophysics 507 (1), L1-L4, 2009
The rotation rates of massive stars: the role of binary interaction through tides, mass transfer, and mergers
SE De Mink, N Langer, RG Izzard, H Sana, A de Koter
The Astrophysical Journal 764 (2), 166, 2013
The VLT-FLAMES Tarantula Survey-VIII. Multiplicity properties of the O-type star population
H Sana, A de Koter, SE de Mink, PR Dunstall, CJ Evans, ...
Astronomy & Astrophysics 550, A107, 2013
Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
I Mandel, SE De Mink
Monthly Notices of the Royal Astronomical Society 458 (3), 2634-2647, 2016
The VLT-FLAMES Tarantula Survey-I. Introduction and observational overview
CJ Evans, WD Taylor, V Hénault-Brunet, H Sana, A de Koter, ...
Astronomy & Astrophysics 530, A108, 2011
The incidence of stellar mergers and mass gainers among massive stars
SE De Mink, H Sana, N Langer, RG Izzard, FRN Schneider
The Astrophysical Journal 782 (1), 7, 2014
Early disc accretion as the origin of abundance anomalies in globular clusters
N Bastian, H Lamers, SE de Mink, SN Longmore, SP Goodwin, M Gieles
Monthly Notices of the Royal Astronomical Society 436 (3), 2398-2411, 2013
Rotational mixing in massive binaries-Detached short-period systems
SE De Mink, M Cantiello, N Langer, OR Pols, I Brott, SC Yoon
Astronomy & Astrophysics 497 (1), 243-253, 2009
The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO
SE De Mink, I Mandel
Monthly Notices of the Royal Astronomical Society 460 (4), 3545-3553, 2016
Rotating massive main-sequence stars-II. Simulating a population of LMC early B-type stars as a test of rotational mixing
I Brott, CJ Evans, I Hunter, A de Koter, N Langer, PL Dufton, M Cantiello, ...
Astronomy & Astrophysics 530, A116, 2011
The effect of stellar rotation on colour–magnitude diagrams: on the apparent presence of multiple populations in intermediate age stellar clusters
N Bastian, SE De Mink
Monthly Notices of the Royal Astronomical Society: Letters 398 (1), L11-L15, 2009
The evolution of runaway stellar collision products
E Glebbeek, E Gaburov, SE De Mink, OR Pols, SFP Zwart
Astronomy & Astrophysics 497 (1), 255-264, 2009
The VLT-FLAMES Tarantula Survey-XII. Rotational velocities of the single O-type stars
OH Ramírez-Agudelo, S Simón-Díaz, H Sana, A de Koter, ...
Astronomy & Astrophysics 560, A29, 2013
Ages of young star clusters, massive blue stragglers, and the upper mass limit of stars: Analyzing age-dependent stellar mass functions
FRN Schneider, RG Izzard, SE de Mink, N Langer, A Stolte, A de Koter, ...
The Astrophysical Journal 780 (2), 117, 2013
The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He ii λ1640 in young star clusters
PA Crowther, SM Caballero-Nieves, KA Bostroem, JM Apellániz, ...
Monthly Notices of the Royal Astronomical Society 458 (1), 624-659, 2016
Efficiency of mass transfer in massive close binaries-Tests from double-lined eclipsing binaries in the SMC
SE De Mink, OR Pols, RW Hilditch
Astronomy & Astrophysics 467 (3), 1181-1196, 2007
Merger rates of double neutron stars and stellar origin black holes: the impact of initial conditions on binary evolution predictions
SE de Mink, K Belczynski
The Astrophysical Journal 814 (1), 58, 2015
Wind Roche-lobe overflow: Application to carbon-enhanced metal-poor stars
C Abate, OR Pols, RG Izzard, SS Mohamed, SE De Mink
Astronomy & Astrophysics 552, A26, 2013
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