Malacaria C, Kretschmar P, Madsen KK, Wilson-Hodge CA, Coley JB, Jenke P, Lutovinov AA, Pottschmidt K, Tsygankov SS, Wilms J (2021)
Publication Type: Journal article
Publication year: 2021
Book Volume: 909
Journal Issue: 2
Accreting X-ray pulsars (XRPs) undergo luminous X-ray outbursts during which the spectral and timing behavior of the neutron star can be studied in detail. We analyze a NuSTAR observation of the XRP XTE J1858+034 during its outburst in 2019. The spectrum is fit with a phenomenological, a semiempirical, and a physical spectral model. A candidate cyclotron line is found at 48 keV, implying a magnetic field of 5.4 x 10(12) G at the site of emission. This is also supported by the physical best-fit model. We propose an orbital period of about 81 days based on the visual inspection of the X-ray outburst recurrence time. Based on Fermi/GBM data, the standard disk accretion-torque theory allowed us to infer a distance of 10.9 1.0 kpc. Pulse profiles are single-peaked and show a pulsed fraction that is strongly energy-dependent at least up to 40 keV.
APA:
Malacaria, C., Kretschmar, P., Madsen, K.K., Wilson-Hodge, C.A., Coley, J.B., Jenke, P.,... Wilms, J. (2021). The X-Ray Pulsar XTE J1858+034 Observed with NuSTAR and Fermi/GBM: Spectral and Timing Characterization plus a Cyclotron Line. Astrophysical Journal, 909(2). https://doi.org/10.3847/1538-4357/abddbc
MLA:
Malacaria, C., et al. "The X-Ray Pulsar XTE J1858+034 Observed with NuSTAR and Fermi/GBM: Spectral and Timing Characterization plus a Cyclotron Line." Astrophysical Journal 909.2 (2021).
BibTeX: Download