Long-term Swift and MAXI observations reveal step-like shifts in Type I outburst orbital phases of GRO J1008-57 that coincide with Type II outbursts, interpreted as cycles of disk depletion and reconstruction.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.
Flux-resolved NuSTAR spectra of 4U 0115+63 show the 10 keV feature maintains constant centroid energy while its flux ratio to the continuum anticorrelates with overall flux, indicating a formation mechanism distinct from both the broadband continuum and the CRSF harmonics.
citing papers explorer
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Temporal evolution of the circumstellar disk orientation in the transient X-ray pulsar GRO J1008-57
Long-term Swift and MAXI observations reveal step-like shifts in Type I outburst orbital phases of GRO J1008-57 that coincide with Type II outbursts, interpreted as cycles of disk depletion and reconstruction.
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Long-term optical variability of high-mass X-ray binaries. III. Polarimetry
Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.
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Flux variability of the "10 keV feature" of 4U 0115+63
Flux-resolved NuSTAR spectra of 4U 0115+63 show the 10 keV feature maintains constant centroid energy while its flux ratio to the continuum anticorrelates with overall flux, indicating a formation mechanism distinct from both the broadband continuum and the CRSF harmonics.