Ronny Blomme | Mark Runacres

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Non-thermal radio emission from O-type stars. III. Is Cygnus OB2 No. 9 a wind-colliding binary?
Non-thermal radio emission from O-type stars. II. HD 167971
Can single O stars produce non-thermal radio emission?
A layered model for non-thermal radio emission from single O stars
An XMM-Newton observation of the multiple system HD 167971 (O5-8V + O5-8V + (O8I)) and the young open cluster NGC 6604
Non-thermal radio emission from O-type stars. I. HD168112
Quasi-simultaneous XMM-Newton and VLA observation of the non-thermal radio emitter HD 168112 (O5.5III(f+))
Non-thermal radio emission from single hot stars
Radio and submillimetre observations of wind structure in zeta Puppis
The memory effect of the ISOPHOT-C100 detector
A multi-wavelength investigation of the non-thermal radio emitting O-star 9 Sgr
An XMM-Newton observation of the Lagoon Nebula and the very young open cluster NGC 6530
Radio and submillimetre observations of epsilon Ori
Stellar Winds of Early-Type Stars
The P32Tools model applied to "staring" observations
ISOPHOT observations of Wolf-Rayet winds
Some peculiarities of the C100 detector
Constraints on Wind Structure from the Infrared and Radio Continuum of Hot Stars
Far Infrared ISO Observations of RD 160529
ISOPHOT Observations of Early-type Stars
The influence of clumping on the infrared and radio continuum of early-type stars
Evidence for clumping from the infrared and radio continuum of hot stars
The infrared and radio continuum of early-type stars
Smooth winds and clumped winds for early-type stars
Smooth winds and clumped winds for early-type stars
The importance of continuum radiation for the stellar wind hydrodynamics of hot stars
The infrared and radio continuum of OB-stars
The infrared excess of early-type stars: modelling the IRAS observations
The infrared excess of early-type stars: using core-halo models for the IRAS observations
Comoving Frame Calculations for LAMBDA-Cephei
Comoving-frame calculations for LAMBDA Cephei