A 500 pc volume-limited sample of hot subluminous stars

HIGHLIGHTS

• What: The aim of these studies was to discern the relative importance of the three main evolutionary channels leading to their formation, and how different combinations of input parameters can alter the resulting population properties. The main motivation behind compiling catalogues of hot subdwarf stars is to constrain evolutionary models. The authors focus initially on the non-composite hot subdwarfs, constituting the primary population in the sample with 257 members . The authors refrain from including them in the analysis presented in this work, and leave it as an open question for future studies as to how they . . .
  

   

  

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