Camiel W. H. de Loore
Structure and evolution of single and binary stars
Evolution of massive stars
Instabilities in luminous early type stars
Wolf-Rayet stars![Characteristic quantities of interest for the studie [sic] of the convection zones in stellar atmospheres](https://s3.amazonaws.com/readfeedstatic/book_covers/thumbnails/rf-placeholder.png)
Characteristic quantities of interest for the studie [sic] of the convection zones in stellar atmospheres- Mechanical energy fluxes generated in the outer convection zones of stellar atmospheres