Positive or negative? The impact of X-ray feedback on the formation of direct collapse black hole seeds

Article, Preprint English OPEN
Regan, John A.; Johansson, Peter H.; Wise, John H.;
(2016)
  • Publisher: Oxford University Press
  • Related identifiers: doi: 10.1093/mnras/stw1307
  • Subject: DARK-MATTER HALOES | 115 Astronomy, Space science | Astrophysics - Astrophysics of Galaxies | stars: Population III | PRIMORDIAL GAS | 1ST STARS | methods: numerical | cosmology: theory | ACCRETION FLOWS | EARLY UNIVERSE | SUPERMASSIVE STARS | VIRIAL TEMPERATURES | HYDROGEN MOLECULES | POPULATION III STARS | GRAVITATIONAL COLLAPSE
    arxiv: Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::High Energy Astrophysical Phenomena | Astrophysics::Galaxy Astrophysics

A nearby source of Lyman-Werner (LW) photons is thought to be a central component in dissociating H-2 and allowing for the formation of a direct collapse black hole seed. Nearby sources are also expected to produce copious amounts of hydrogen ionizing photons and X-ray ... View more
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