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  • 1
    Electronic Resource
    Electronic Resource
    The black flash model of QSOs (1978)
    Springer
    General relativity and gravitation 9 (1978), S. 189-193 
    Details
    ISSN: 1572-9532
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract A model for QSOs and the nuclei of Seyfert Galaxies is proposed in which mass lost from stars in a galactic nucleus repeatedly builds to a critical density and then collapses to the center where it accretes onto a massive black hole (≈108 M ⊙), emitting great luminosity. This model describes a means of starting with an ordinary nucleus and developing conditions found in QSOs. By invoking intermittent flashes we overcome a difficulty previously encountered in similar models in which plausible sources of mass in reasonable galactic nuclei fail by a factor of ≈10−2 in fueling a black hole at QSO luminosities.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00759373
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