Raymond Lyttleton (1911-95)

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Hoyle–Lyttleton Accretion onto Accretion Disks

We investigate Hoyle–Lyttleton accretion for the case where the central source is a luminous accretion disk. In classical Hoyle-Lyttleton accretion onto a “spherical” source, accretion takes place in an axially symmetric manner around a so-called accretion axis. In the spherical case the accretion rate Ṁ is given as ṀHL(1− Γ), where ṀHL is the accretion rate of the classical Hoyle–Lyttleton acc...

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ژورنال

عنوان ژورنال: Nature

سال: 1995

ISSN: 0028-0836,1476-4687

DOI: 10.1038/375738a0