| The outer evolution of instability-generated structure in radiatively driven stellar winds MC Runacres, SP Owocki Astronomy & Astrophysics 381 (3), 1015-1025, 2002 | 234 | 2002 |
| A pseudo-planar, periodic-box formalism for modelling the outer evolution of structure in spherically expanding stellar winds MC Runacres, SP Owocki Astronomy & Astrophysics 429 (1), 323-333, 2005 | 75 | 2005 |
| A multi-wavelength investigation of the non-thermal radio emitting O-star 9 Sgr G Rauw, R Blomme, WL Waldron, MF Corcoran, JM Pittard, AMT Pollock, ... Astronomy & Astrophysics 394 (3), 993-1008, 2002 | 61 | 2002 |
| An-observation of the Lagoon Nebula and the very young open cluster NGC 6530 G Rauw, Y Nazé, E Gosset, IR Stevens, R Blomme, MF Corcoran, ... Astronomy & Astrophysics 395 (2), 499-513, 2002 | 58 | 2002 |
| Can single O stars produce non-thermal radio emission? S Van Loo, MC Runacres, R Blomme Astronomy & Astrophysics 452 (3), 1011-1019, 2006 | 50 | 2006 |
| Radio and submillimetre observations of ϵ Ori R Blomme, RK Prinja, MC Runacres, S Colley Astronomy & Astrophysics 382 (3), 921-934, 2002 | 45 | 2002 |
| Experimental validation of the power enhancement of a pair of vertical-axis wind turbines A Vergaerde, T De Troyer, L Standaert, J Kluczewska-Bordier, D Pitance, ... Renewable Energy 146, 181-187, 2020 | 43 | 2020 |
| Non-thermal radio emission from O-type stars-III. Is Cygnus OB2 No. 9 a wind-colliding binary? S Van Loo, R Blomme, SM Dougherty, MC Runacres Astronomy & Astrophysics 483 (2), 585-590, 2008 | 42 | 2008 |
| Effect of turbulence on the performance of VAWTs: An experimental study in two different wind tunnels AC Molina, T De Troyer, T Massai, A Vergaerde, MC Runacres, G Bartoli Journal of Wind Engineering and Industrial Aerodynamics 193, 103969, 2019 | 41 | 2019 |
| Experimental characterisation of the wake behind paired vertical-axis wind turbines A Vergaerde, T De Troyer, S Muggiasca, I Bayati, M Belloli, ... Journal of Wind Engineering and Industrial Aerodynamics 206, 104353, 2020 | 37 | 2020 |
| The infrared and radio continuum of early-type stars. MC Runacres, R Blomme Astronomy and Astrophysics, v. 309, p. 544-557 309, 544-557, 1996 | 37 | 1996 |
| Quasi-simultaneous XMM-Newton and VLA observation of the non-thermal radio emitter HD 168112 (O5. 5III (f)) M De Becker, G Rauw, R Blomme, WL Waldron, H Sana, JM Pittard, ... Astronomy & Astrophysics 420 (3), 1061-1077, 2004 | 36 | 2004 |
| Non-thermal radio emission from O-type stars-II. HD 167971 R Blomme, M De Becker, MC Runacres, S Van Loo, DYAS Gunawan Astronomy & Astrophysics 464 (2), 701-708, 2007 | 34 | 2007 |
| Non-thermal radio emission from O-type stars-I. HD 168112 R Blomme, S Van Loo, M De Becker, G Rauw, MC Runacres, ... Astronomy & Astrophysics 436 (3), 1033-1040, 2005 | 32 | 2005 |
| Reliability‐based design optimization of computation‐intensive models making use of response surface models G Steenackers, R Versluys, M Runacres, P Guillaume Quality and Reliability Engineering International 27 (4), 555-568, 2011 | 31 | 2011 |
| An XMM-Newton observation of the multiple system HD 167971 (O5-8V+ O5-8V+(O8I)) and the young open cluster NGC 6604 M De Becker, G Rauw, R Blomme, JM Pittard, IR Stevens, MC Runacres Astronomy & Astrophysics 437 (3), 1029-1046, 2005 | 31 | 2005 |
| A layered model for non-thermal radio emission from single O stars S Van Loo, MC Runacres, R Blomme Astronomy & Astrophysics 433 (1), 313-322, 2005 | 30 | 2005 |
| Radio and submillimetre observations of wind structure in ζ Puppis R Blomme, RK Prinja, MC Runacres, JS Clark Astronomy & Astrophysics 408 (2), 715-727, 2003 | 30 | 2003 |
| Non-thermal radio emission from single hot stars S Van Loo, MC Runacres, R Blomme Astronomy & Astrophysics 418 (2), 717-725, 2004 | 27 | 2004 |
| The influence of clumping on the infrared and radio continuum of early-type stars. R Blomme, MC Runacres Astronomy and Astrophysics, v. 323, p. 886-900 323, 886-900, 1997 | 25 | 1997 |
Tim De TroyerProfessor of Aeronautical Engineering, Vrije Universiteit BrusselGeverifieerd e-mailadres voor vub.ac.be
