On Monolithic Supermassive Stars

23 Mar 2020 Woods Tyrone E. Heger Alexander Haemmerlé Lionel

Supermassive stars have been proposed as the progenitors of the massive ($\sim 10^{9}\,\rm{M}_{\odot}$) quasars observed at $z\sim7$. Prospects for directly detecting supermassive stars with next-generation facilities depend critically on their intrinsic lifetimes, as well as their formation rates... (read more)

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Categories


  • ASTROPHYSICS OF GALAXIES
  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • SOLAR AND STELLAR ASTROPHYSICS