Abstract
The unusual properties of the bursting X-ray pulsar GRO J1744-28 are explained interms of a low-mass X-ray binary system consisting of an evolvedstellar companion transferring mass through Roche-lobe overflow onto aneutron star, implying that the inclination of the system is < 1 is acorrection factor that depends on the orientation of the neutron star.
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CITATION STYLE
APA
Sturner, S. J., & Dermer, C. D. (1996). On the Nature of the Bursting X-Ray Pulsar GRO J1744−28. The Astrophysical Journal, 465(1), L31–L34. https://doi.org/10.1086/310126
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