천문학회지 (Journal of The Korean Astronomical Society)
- 제29권spc1호
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- Pages.235-236
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- 1996
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- 1225-4614(pISSN)
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- 2288-890X(eISSN)
THEORETICAL LINE PROFILES OF THE MAGNETIC COMPACT STARS
초록
Using a phenomenological model for the accretion onto the magnetic white dwarf, we calclliated some optical line profiles from the magnetosphere of such systems. Line profiles of these systems seem to be produced in the magnetosphere of the compact star due to the reemission of X-ray produced near the stellar surface. Some results of our new calculation and the analysis of these results will be presented. Our results show that the model used here can reproduce the observed optical line profiles and open the possiblity to determine the parameters of individual systems.