Shared accretion mechanism for X-ray binaries.
X-ray binaries are systems comprising a normal star and a collapsed star — a neutron star or a black hole. Matter falling from the normal star to the collapsed star becomes so hot that it emits copious X-rays.
When the luminosity of these X-rays is high, the instabilities that occur can help us to understand the extreme conditions found in the vicinity of collapsed stars. One such high-luminosity source is the black hole GRS 1915+105, which shows curious variations in signals at X-ray and radio frequencies
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