FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1969578278> ?p ?o ?g. }

• W1969578278 endingPage "871" @default.
• W1969578278 startingPage "858" @default.
• W1969578278 abstract "We have used the hydrodynamical adaptive mesh refinement code enzo to investigate the dynamical evolution of the gas at the centre of dark matter haloes with virial velocities of ∼20−30 km s−1 and virial temperatures of ∼13 000–30 000 K at z∼ 15 in a cosmological context. The virial temperature of the dark matter haloes is above the threshold where atomic cooling by hydrogen allows the gas to cool and collapse. We neglect cooling by molecular hydrogen and metals, as may be plausible if H2 cooling is suppressed by a metagalactic Lyman–Werner background or an internal source of Lyman–Werner photons, and metal enrichment has not progressed very far. The gas in the haloes becomes gravitationally unstable and develops turbulent velocities comparable to the virial velocities of the dark matter haloes. Within a few dynamical times, it settles into a nearly isothermal density profile over many decades in radius losing most of its angular momentum in the process. About 0.1–1 per cent of the baryons, at the centre of the dark matter haloes, collapse into a self-gravitating, fat, ellipsoidal, centrifugally supported exponential disc with scalelength of ∼0.075–0.27 pc and rotation velocities of 25–60 km s−1. We are able to follow the settling of the gas into centrifugal support and the dynamical evolution of the compact disc in each dark matter halo for a few dynamical times. The dynamical evolution of the gas at the centre of the haloes is complex. In one of the haloes, the gas at the centre fragments into a triple system leading to strong tidal perturbations and eventually to the infall of a secondary smaller clump into the most massive primary clump. The formation of centrifugally supported self-gravitating massive discs is likely to be an important intermediary stage en route to the formation of a massive black hole seed." @default.
• W1969578278 created "2016-06-24" @default.
• W1969578278 creator A5039809051 @default.
• W1969578278 creator A5046966092 @default.
• W1969578278 date "2009-03-01" @default.
• W1969578278 modified "2023-10-16" @default.
• W1969578278 title "The formation of compact massive self-gravitating discs in metal-free haloes with virial temperatures of ∼13 000-30 000 K" @default.
• W1969578278 cites W1651289634 @default.
• W1969578278 cites W1672666614 @default.
• W1969578278 cites W1821429365 @default.
• W1969578278 cites W1892333491 @default.
• W1969578278 cites W1964280853 @default.
• W1969578278 cites W1975059575 @default.
• W1969578278 cites W197783772 @default.
• W1969578278 cites W1978186191 @default.
• W1969578278 cites W1993132186 @default.
• W1969578278 cites W1994998672 @default.
• W1969578278 cites W1996131714 @default.
• W1969578278 cites W2005631644 @default.
• W1969578278 cites W2011393937 @default.
• W1969578278 cites W2018681307 @default.
• W1969578278 cites W2019473452 @default.
• W1969578278 cites W2024319723 @default.
• W1969578278 cites W2024486982 @default.
• W1969578278 cites W2027765267 @default.
• W1969578278 cites W2031670668 @default.
• W1969578278 cites W2040912209 @default.
• W1969578278 cites W2050931690 @default.
• W1969578278 cites W2060304114 @default.
• W1969578278 cites W2061068883 @default.
• W1969578278 cites W2065201732 @default.
• W1969578278 cites W2070803987 @default.
• W1969578278 cites W2073510197 @default.
• W1969578278 cites W2077047259 @default.
• W1969578278 cites W2079349557 @default.
• W1969578278 cites W2081092366 @default.
• W1969578278 cites W2083592770 @default.
• W1969578278 cites W2083870045 @default.
• W1969578278 cites W2086028003 @default.
• W1969578278 cites W2087432755 @default.
• W1969578278 cites W2093316516 @default.
• W1969578278 cites W2101568531 @default.
• W1969578278 cites W2118265220 @default.
• W1969578278 cites W2120036169 @default.
• W1969578278 cites W2129495060 @default.
• W1969578278 cites W2133678282 @default.
• W1969578278 cites W2133778146 @default.
• W1969578278 cites W2134253073 @default.
• W1969578278 cites W2135894620 @default.
• W1969578278 cites W2136969532 @default.
• W1969578278 cites W2150173609 @default.
• W1969578278 cites W2151133271 @default.
• W1969578278 cites W2160005867 @default.
• W1969578278 cites W2162475780 @default.
• W1969578278 cites W2168231518 @default.
• W1969578278 cites W2953087527 @default.
• W1969578278 cites W3023613093 @default.
• W1969578278 cites W3098575376 @default.
• W1969578278 cites W3101092402 @default.
• W1969578278 cites W3101409234 @default.
• W1969578278 cites W3103144563 @default.
• W1969578278 cites W3103440046 @default.
• W1969578278 cites W3105082704 @default.
• W1969578278 cites W3105161400 @default.
• W1969578278 cites W3105643723 @default.
• W1969578278 cites W3122860981 @default.
• W1969578278 cites W3125077931 @default.
• W1969578278 cites W3125275757 @default.
• W1969578278 cites W4382891143 @default.
• W1969578278 doi "https://doi.org/10.1111/j.1365-2966.2008.14088.x" @default.
• W1969578278 hasPublicationYear "2009" @default.
• W1969578278 type Work @default.
• W1969578278 sameAs 1969578278 @default.
• W1969578278 citedByCount "88" @default.
• W1969578278 countsByYear W19695782782012 @default.
• W1969578278 countsByYear W19695782782013 @default.
• W1969578278 countsByYear W19695782782014 @default.
• W1969578278 countsByYear W19695782782015 @default.
• W1969578278 countsByYear W19695782782016 @default.
• W1969578278 countsByYear W19695782782017 @default.
• W1969578278 countsByYear W19695782782018 @default.
• W1969578278 countsByYear W19695782782019 @default.
• W1969578278 countsByYear W19695782782020 @default.
• W1969578278 countsByYear W19695782782021 @default.
• W1969578278 countsByYear W19695782782022 @default.
• W1969578278 countsByYear W19695782782023 @default.
• W1969578278 crossrefType "journal-article" @default.
• W1969578278 hasAuthorship W1969578278A5039809051 @default.
• W1969578278 hasAuthorship W1969578278A5046966092 @default.
• W1969578278 hasBestOaLocation W19695782781 @default.
• W1969578278 hasConcept C121332964 @default.
• W1969578278 hasConcept C125857072 @default.
• W1969578278 hasConcept C151730666 @default.
• W1969578278 hasConcept C159249277 @default.
• W1969578278 hasConcept C184665706 @default.
• W1969578278 hasConcept C189549420 @default.
• W1969578278 hasConcept C206564472 @default.
• W1969578278 hasConcept C2779343474 @default.

• next