Spectrum formation in X-ray pulsars at very low mass accretion rate: Monte Carlo approach

Author(s):
Mushtukov, A.A.; Suleimanov, V.F.; Tsygankov, S.S.; Portegies Zwart, S.F. (0000-0001-5839-0302)
Published
2021
Publication type
Article / Letter to editor
PolarizationRadiative transferScatteringStars: magnetic fieldStars: neutronX-rays: binariesAstrophysics - high energy astrophysical phenomena
Date issued
2021
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2021), Vol. 503, no. 4, p. 5193-5203
hdl
1887/3256720
doi
10.1093/mnras/stab811
URL
https://ui.adsabs.harvard.edu/abs/2021MNRAS.503.5193M