Constraints on the pairing properties of main-sequence stars from observations of white dwarfs in binary systems
Observations of main-sequence stars conducted over the last several decades have clearly shown that something like 50 per cent of stars of spectral types G and F occur in multiple systems. For earlier spectral types, the incidence of multiplicity is even
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Ferrario_Constraints_on_the_pairing_2012.pdf||354.68 kB||Adobe PDF|
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