• Extremely low-mass white dwarfs in interacting binary systems 

      Soethe, Leonardo Taynô Tosetto (2021) [Tese]
      Extremely low-mass white dwarfs (ELM WDs) are understood to be the result of binary evolution in which a low-mass donor star — mass of the order of that of the Sun — is stripped by its companion, leaving behind a helium-core ...
    • White dwarf and subdwarf stars in the sloan digital sky survey 

      Pelisoli, Ingrid Domingos (2018) [Tese]
      White dwarf stars are the final observable evolutionary state of over 95% of stars and also a common outcome in binary evolution. Therefore, studying white dwarfs is a powerful tool to understand both single and binary ...