Simulations show wide primordial binaries are disrupted as efficiently as if no binaries formed, while close binaries survive, indicating close and equal-mass binary properties are imprinted at the star formation stage.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
SIRIUS Project: Dynamical Evolution of Primordial Binaries during Star Cluster Formation
Simulations show wide primordial binaries are disrupted as efficiently as if no binaries formed, while close binaries survive, indicating close and equal-mass binary properties are imprinted at the star formation stage.