Massive stars in the small magellanic cloud – evolution, rotation, and surface abundances

HIGHLIGHTS

• who: Bouret J.-C. and collaborators from the (UNIVERSITY) have published the article: Massive stars in the Small Magellanic Cloud - Evolution, rotation, and surface abundances, in the Journal: (JOURNAL)
• what: For the purpose of the analysis, the authors would preferably only work with single stars. The main reason is that predictions of the surface chemical patterns resulting from binary evolution are still very uncertain (see Langer 2012, for a review). In Fig 2 the authors show the location of the individual stars in the classical HRD (top) and in the Kiel diagram (KD, bottom). In . . .
  

   

  

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