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The study investigates the orbital period modulation of the symbiotic X-ray binary GX 1+4 using X-ray observations from various telescopes. The authors apply Lomb-Scargle and epoch-folding methods to analyze light curves and spin-frequency data, confirming a previously suggested orbital period of approximately 1161 days. Their findings indicate a high inclination of the orbital plane and provide constraints on the neutron star

Author

jldirac

Language

EN