Forming Pop III binaries in self-gravitating discs: how to keep the orbital angular momentum
Sign Up to like & getrecommendations! Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz1824
Abstract: The disc fragmentation is a possible process leading to the formation of Population III stellar binary systems. However, numerical simulations show diverse fates of the fragments; some evolve into stable binaries and others merge away… read more here.
Keywords: angular momentum; forming pop; self gravitating; orbital angular ... See more keywords