A nearly coplanar Be star disk in a circular-orbit binary can become eccentric via the 3:1 Lindblad resonance, producing type I outbursts when the neutron star passes the disk apastron.
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Type I outbursts in low eccentricity Be/X-ray binaries
A nearly coplanar Be star disk in a circular-orbit binary can become eccentric via the 3:1 Lindblad resonance, producing type I outbursts when the neutron star passes the disk apastron.