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What is Cyclotron Absorption in SMC X-2 Outburst about?

This study presents the spectral and temporal properties of the Be/X-ray binary pulsar SMC X-2 during its 2015 and 2022 outbursts, highlighting a unique pulse profile that evolves with luminosity. The analysis indicates a spectral transition from sub-critical to supercritical regimes and an increase in cyclotron line energy from 29.5 keV in 2015 to 31.5 keV in 2022. The findings suggest that the observed variations in cyclotron line energy may be due to accretion-induced screening or geometrical changes in

Author

impetus909

Language

EN