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.
Accretion Disks
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
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).
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
QPO signatures of disk restoration after type-I X-ray bursts from 4U~1636$-$536
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.