The first so - called helium nova, the possible result of a large white dwarf sucking material from a hydrogen -
deficient companion star, may be a precursor to a supernova
HD 147513 A is a so - called young «Barium dwarf» (s - process element rich but comparatively carbon
deficient)
star that was probably enriched by an asymptotic branch giant (AGB)
star (see Gacrux) but is now a very dim, white dwarf
companion, which has an observed separation of around 4,400 AUs — 5.7» at a HIPPARCOS distance estimate of 42.0 ly (Porto de Mello and da Silva, 1997; and Poveda et al, 1993, pp. 74 - 75).