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تسجيل مستخدم جديدInsight-HXMT observations of Swift J0243.6+6124 during its 2017-2018 outburst
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The recently discovered neutron star transient Swift J0243.6+6124 has been monitored by {it the Hard X-ray Modulation Telescope} ({it Insight-rm HXMT). Based on the obtained data, we investigate the broadband spectrum of the source throughout the outburst. We estimate the broadband flux of the source and search for possible cyclotron line in the broadband spectrum. No evidence of line-like features is, however, found up to $rm 150~keV$. In the absence of any cyclotron line in its energy spectrum, we estimate the magnetic field of the source based on the observed spin evolution of the neutron star by applying two accretion torque models. In both cases, we get consistent results with $Brm sim 10^{13}~G$, $Drm sim 6~kpc$ and peak luminosity of $rm >10^{39}~erg~s^{-1}$ which makes the source the first Galactic ultraluminous X-ray source hosting a neutron star.
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We report on analysis of observations of the bright transient X-ray pulsar src obtained during its 2017-2018 giant outburst with Insight-HXMT, emph{NuSTAR}, and textit{Swift} observatories. We focus on the discovery of a sharp state transition of the
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This paper reports on the X-ray emission evolution of the ultra-luminous Galactic X-ray pulsar, Swift J0243.6+6124, during the 2017-2018 giant outburst observed by the MAXI GSC. The 2-30 keV light curve and the energy spectra confirm that the luminos
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