A strongly truncated inner accretion disk in the Rapid Burster
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Peer-reviewed
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The neutron star (NS) low-mass X-ray binary (LMXB) the Rapid Burster (RB; MXB 1730-335) uniquely shows both Type I and Type II X-ray bursts. The origin of the latter is ill-understood but has been linked to magnetospheric gating of the accretion flow. We present a spectral analysis of simultaneous
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1745-3933
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European Research Council (340442)
European Commission (627148)