2 citations · 5 across the 5 of their papers we have counts for
5 papers · 1 filter
On the origin of microturbulence in hot stars
M. Cantiello, N. Langer, I. Brott +5
We present results from the first extensive study of convection zones in the envelopes of hot massive stars, which are caused by opacity peaks associated with iron and helium ioniz…
Rotational Mixing in Magellanic Clouds B Stars - Theory versus Observation
I. Brott, I. Hunter, A. de Koter +3
We have used VLT FLAMES data to constrain the uncertain physics of rotational mixing in stellar evolution models. We have simulated a population of single stars and find two groups…
Probing the Early Evolution of Young High-Mass Stars
E. Puga, A. Bik, L. B. M. F. Waters +22
Near-infrared imaging surveys of high-mass star-forming regions reveal an amazingly complex interplay between star formation and the environment (Churchwell et al. 2006; Alvarez et…
Advances in mass-loss predictions
Jorick S. Vink, P. Benaglia, B. Davies +2
We present the results of Monte Carlo mass-loss predictions for massive stars covering a wide range of stellar parameters. We critically test our predictions against a range of obs…
Pre-supernova mass loss predictions for massive stars
Jorick S. Vink, Alex de Koter, Rubina Kotak
Massive stars and supernovae (SNe) have a huge impact on their environment. Despite their importance, a comprehensive knowledge of which massive stars produce which SNe is hitherto…