Accretion Disks

D-85740 Garching; Germany); H.C. Spruit (Max Planck Institute for Astrophysics; P.O. Box 1523

Accretion Disks

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arxiv astro-ph/9502098 v1 pith:VWY2OANW submitted 1995-02-26 astro-ph

H.C. Spruit (Max Planck Institute for Astrophysics , P.O. Box 1523 , D-85740 Garching , Germany) This is my paper · ORCID

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keywords accretionalparappearedaspectsbinariescataclysmiccorrectsdisk

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This is an introduction to accretion disk theory, with emphasis on aspects relevant for X-ray Binaries and Cataclysmic Variables. The text corrects some mistakes in an earlier version, which appeared in 'Lives of Neutron Stars', A. Alpar, \"U. Kizilo\u glu and J. van Paradijs (eds.), Kluwer, Dordrecht (NATO ASI series, 1994).

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Cited by 1 Pith paper

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QPO signatures of disk restoration after type-I X-ray bursts from 4U~1636$-$536
astro-ph.HE 2025-05 conditional novelty 4.0 of 10

In three bursts of 4U 1636-536, kHz QPOs are absent for 100-200 s after a Type-I burst and return around 200 s, suggesting temporary inner disk disruption and viscous restoration.

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