SIMBAD references

2020ApJ...896..124S - Astrophys. J., 896, 124-124 (2020/June-3)

X-ray emission evolution of the Galactic ultraluminous X-ray pulsar Swift J0243.6+6124 during the 2017-2018 outburst observed by the MAXI GSC.

SUGIZAKI M., OEDA M., KAWAI N., MIHARA T., MAKISHIMA K. and NAKAJIMA M.

Abstract (from CDS):

This paper reports on the X-ray emission evolution of the ultraluminous Galactic X-ray pulsar Swift J0243.6+6124 during the giant outburst from 2017 October to 2018 January as observed by the MAXI GSC all-sky survey. The 2-30 keV light curve and the energy spectra confirm the source luminosity LX assuming an isotropic emission reached 2.5 x 1039 erg s–1, 10 times higher than the Eddington limit for a 1.4 M neutron star. When the source was luminous with LX >= 0. 9 x 1038 erg s–1, it generally exhibited a negative correlation on a hardness-intensity diagram. However, two hardness ratios, a soft color (=4-10 keV/2-4 keV) and a hard color (=10-20 keV/4-10 keV), showed somewhat different behavior across a characteristic luminosity of Lc ≃ 5 x 1038 erg s–1. The soft color changed more than the hard color when LX < Lc, whereas the opposite was observed above Lc. The spectral change above Lc was represented by a broad enhanced feature at ∼6 keV on top of the canonical cutoff power-law continuum. The pulse profiles, derived daily, made the transition from a single-peak to a double-peak as the source brightened across Lc. These spectral and pulse-shape properties can be interpreted by a scenario in which the accretion columns on the neutron-star surface, producing the Comptonized X-ray emission, gradually became taller as LX increases. The broad 6 keV enhancement could be a result of cyclotron-resonance absorption at ∼10 keV, corresponding to a surface magnetic field Bs ≃ 1.1 x 1012 G. The spin-frequency derivatives calculated with the Fermi GBM data showed a smooth positive correlation with LX up to the outburst peak, and its linear coefficient is comparable to those of typical Be binary pulsars whose Bs are (1-8) x 1012 G. These results suggest that the Bs of Swift J0243.6+6124 is a few times 1012 G.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Neutron stars - Binary pulsars - Accretion - High mass x-ray binary stars

VizieR on-line data: <Available at CDS (J/ApJ/896/124): fig1.dat>

Simbad objects: 18

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2023.02.04-10:57:05

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