Disc fragmentation and intermittent accretion on to supermassive stars
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DOI: 10.1093/mnras/staa3462
Abstract: Supermassive stars (SMSs) with $\sim10^{4-5}~\mathrm{M}_{\odot}$ are candidate objects for the origin of supermassive black holes observed at redshift $z$>6. They are supposed to form in primordial-gas clouds that provide the central stars with gas at… read more here.
Keywords: fragmentation intermittent; supermassive stars; accretion; disc fragmentation ... See more keywords