Origin of the X-ray off-states in Vela X-1
A. Manousakis, R. Walter

TL;DR
This study uses hydrodynamic simulations to explain Vela X-1's X-ray off-states and variability, showing that instabilities in the stellar wind flow can account for observed phenomena without invoking more complex mechanisms.
Contribution
The paper demonstrates that hydrodynamic instabilities alone can reproduce Vela X-1's X-ray variability, challenging the necessity of clumpy winds or magnetic gating explanations.
Findings
Simulated off-states last 5-120 minutes, matching observations.
Oscillations in accretion rate occur with a period of about 6800 seconds.
Flares up to 10^{37} erg/s are produced in simulations.
Abstract
: Vela X-1 is the prototype of the classical sgHMXB systems. Recent continuous and long monitoring campaigns revealed a large hard X-rays variability amplitude with strong flares and off-states. This activity has been interpreted invoking clumpy stellar winds and/or magnetic gating mechanisms. : We are probing if the observed behaviour could be explained by unstable hydrodynamic flows close to the neutron star rather than the more exotic phenomena. : We have used the hydrodynamic code VH-1 to simulate the flow of the stellar wind with high temporal resolution and to compare the predicted accretion rate with the observed light-curves. : The simulation results are similar to the observed variability. Off-states are predicted with a duration of 5 to 120 minutes corresponding to transient low density bubbles forming around the neutron star.…
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