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Very low-metallicity massive stars:
Free accessPre-SN evolution models and primary nitrogen productionEDP Sciences | 2007| -
The GSF instability and turbulence do not account for the relatively low rotation rate of pulsars
Online Contents | 2010| -
The GSF instability and turbulence do not account for the relatively low rotation rate of pulsars
Online Contents | 2010| -
The GSF instability and turbulence do not account for the relatively low rotation rate of pulsars
Free accessEDP Sciences | 2010| -
The Evolution of Massive Stars in the Context of V838 Monocerotis
British Library Conference Proceedings | 2007| -
Very low-metallicity massive stars: Pre-SN evolution models and primary nitrogen production
British Library Online Contents | 2007| -
Rotating Massive Stars @ Very Low Z: High C & N Production
British Library Conference Proceedings | 2006| -
Rotating massive stars: Pre#8211SN models and stellar yields at solar metallicity
Online Contents | 2005| -
Constraining transport of angular momentum in stars
Free accessCombining asteroseismic observations of core helium burning stars and white dwarfsEDP Sciences | 2019| -
Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars
American Institute of Physics | 2016|
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