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The Astrophysical journal, ISSN 0004-637X, 06/2015, Volume 806, Issue 2, pp. 164 - 8
.... To form an accretion flow, the bound matter must lose a significant amount of energy, with the actual amount depending on the characteristic scale of the flow measured... 
black hole physics | stars: black holes | galaxies: nuclei | accretion, accretion disks | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Accretion | Heating | Luminosity | Black holes (astronomy) | Nuclear power generation | Formations | Disruption | Accretion disks
Journal Article
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 07/2007, Volume 469, Issue 3, pp. 811 - 828
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2012, Volume 420, Issue 1, pp. 416 - 429
We show that discs accreting on to the magnetosphere of a rotating star can end up in a trapped state, in which the inner edge of the disc stays near the corotation radius, even at low and varying accretion rates... 
stars: formation | stars: magnetic field | stars: oscillations | accretion, accretion discs | instabilities | stars: rotation | Stars: magnetic field | Instabilities | Stars: formation | Accretion, accretion discs | Stars: oscillations | Stars: rotation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Geomagnetism | Magnetosphere | Astronomy | Magnetic fields | Accretion disks
Journal Article