천문학회지 (Journal of The Korean Astronomical Society)
- 제27권1호
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- Pages.45-53
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- 1994
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- 1225-4614(pISSN)
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- 2288-890X(eISSN)
MONTE CARLO SIMULATION OF COMPTONIZATION IN A SPHERICAL SHELL GEOMETRY
- SEON KWANG IL (Department of Physics, Korea Advanced Institute of Science and Technology) ;
- MIN KYOUNG WOOK (Department of Physics, Korea Advanced Institute of Science and Technology) ;
- CHOI CHUL SUNG (Korea Astronomy Observatory) ;
- NAM UK WON (Korea Astronomy Observatory)
- 발행 : 1994.04.01
초록
We present the calculation of X -ray spectra produced through Compton scattering of soft X-rays by hot electrons in the spherical shell geometry, using fully relativistic Monte Carlo simulation. With this model, we show that the power-law component, which has been observed in the low luminosity state of low-mass X-ray binaries (LMXBs), is explained physically. From a spectral. analysis, we find that spectral hardness is mainly due to the relative contribution of scattered component. In addition, we see that Wi en spectral features appear when the plasma is optically thick, especially in the high energy range,