Abstract
The X-ray binary GX301-2 was observed extensively by the Tenma satellite. GX301-2 exhibits strong fluorescent iron line emission and a strong K-edge absorption feature. Time variations in the X-ray luminosity, absorption column density, and the iron emission line are used to study the properties of the circumstellar matter in this system.
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© 1991 Springer-Verlag
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Leahy, D.A. (1991). Properties of iron line emission in the X-ray binary GX301-2. In: Treves, A., Perola, G.C., Stella, L. (eds) Iron Line Diagnostics in X-ray Sources. Lecture Notes in Physics, vol 385. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0031282
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DOI: https://doi.org/10.1007/BFb0031282
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