refereed journal papers

conference papers

preprints and others

• Non-thermal radio emission from O-type stars III. Is Cyg OB2 No. 9 a wind-colliding binary?
  Van Loo, S. Blomme, R., Dougherty, S. M., & Runacres, M. C., A & A, 483, 585

• The effect of ambipolar resistivity on the formation of dense cores. [pdf]
  Van Loo, S., Falle, S. A. E. G., Hartquist, T. W., & Barker, A. J., A & A, 484, 275

• Schock-triggered formation of magnetically-dominated clouds [pdf]
  Van Loo, S., Falle, S. A. E. G., Hartquist, T. W. & Moore, T. J. T. 2007, A & A, 471, 213

• Dense core compression and fragmentation induced by the scattering
  of hydromagnetic waves [pdf]
  Van Loo, S., Falle, S. A. E. G. & Hartquist, T. W. 2007, MNRAS, 376, 779

• Non-thermal radio emission from O-type stars II. HD 167971 [pdf]
  Blomme, R., De Becker, M., Runacres, M. C., Van Loo, S.,
  & Setia Gunawan, D. Y. A., 2007, A & A, 464, 701

• XMM-Newton observations of the massive colliding wind binary and
  non-thermal radio emitter Cyg OB2 No. 8A (O6If + O5.5III(f)) [pdf]
  De Becker, M., Rauw, G., Sana, H., Pollock, A. M. T., Pittard, J. M., Blomme, R.,
  Stevens, I. R., & Van Loo, S. 2006, MNRAS, 371, 1280

• Generation of density inhomogeneities by magnethydrodynamic waves
  in two dimensions [pdf]
  Van Loo, S., Falle, S. A. E. G. & Hartquist, T. W. 2006, MNRAS, 370, 975

• Can single O stars produce non-thermal radio emission? [pdf]
  Van Loo, S., Runacres, M. C., & Blomme, R. 2006, A & A, 452, 1011

• Non-thermal radio emission from O-type stars. I. HD168112 [pdf]
  Blomme, R., Van Loo, S., De Becker, M., Rauw, G., Runacres, M.C.,
  Setia Gunawan, D. Y. A., & Chapman, J. M. 2005, A & A 436, 1033

• A layered model for non-thermal radio emission from single hot stars [pdf]
  Van Loo, S., Runacres, M. C., & Blomme, R. 2005, A & A 433, 313

• Quasi-simultaneous XMM-Newton and VLA observations of the
  non-thermal radio emitter HD 168112 (O5.5III(f+)) [pdf]
  De Becker, M., Rauw, G., Blomme, R., Waldron, W. L., Sana, H., Pittard, J. M.,
  Eenens, P., Stevens, I. R., Runacres, M. C., Van Loo, S. & Pollock, A. M. T.
  2004, A & A 420, 1061

• Non-thermal radio emission from single hot stars [pdf]
  Van Loo, S., Runacres, M. C., & Blomme, R. 2004, A & A 418, 717

• A multi-wavelength investigation of the non-thermal radio emitting
  O-star 9 Sgr [pdf]
  Rauw, G., Blomme, R., Waldron, W. L., Corcoran, M. F., Pittard, J. M.,
  Pollock, A. M. T., Runacres, M. C., Sana, H., Stevens, I. R., & Van Loo, S.
  2002, A & A 394, 993

• Dust in interstellar clouds, evolved stars and supernovae [pdf]
  Hartquist, T. W., Van Loo, S., Falle, S. A. E. G., Caselli, P., & Ashmore, I. in "Fifth international
  Conference on the physics of dusty plasmas."; AIPC 1041, 2008, 101

• Are all non-thermal radio-emitting O stars binaries? [pdf]
  Van Loo, S. in "Active OB stars: Laboratories for Stellar and Circumstellar Physics";
  ASP Conference Series 361, 2007, 515

• The generation of large and small-scale structure by magnetosonic waves [pdf]
  Van Loo, S., Falle, S. A. E. G. & Hartquist, T. W. in "Triggered Star Formation
  in a Turbulent ISM", Proceedings of IAUS 237, 2006, 160

• The generation of structure in molecular clouds by MHD waves [pdf]
  Van Loo, S., Falle, S. A. E. G. & Hartquist, T. W. in Proceedings of
  "Interaction of Stars with their Environment III", 2006

• Can single O stars produce non-thermal radio emission?
  Or are they binaries [pdf]
  Van Loo, S. in "Massive stars and High-Energy Emission in OB associations";
  Proceedings of JENAM 2005, 61

• Non-thermal radio emission from single hot stars [pdf]
  Van Loo, S. in "Winds, Bubbles and Explosions: a Conference to honor John Dyson";
  2003, RevMexAA 15, 230

• Non-thermal radio emission from single O stars [pdf]
  Van Loo, S. in Meeting of the Workgroup Extended Atmospheres;
  2002, JAD 8S, 8

• Non-thermal radio emission from single hot stars [pdf]
  Van Loo, S. 2005, PhD thesis Katholieke Universiteit Leuven

• Non-thermal radio emission from O stars: binary versus single [pdf]
  Van Loo, S. in "Massive Stars in Interacting Binaries"; in press