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- W2135893120 abstract "We present a systematic study of GX 339−4 in both its very high and low hard states from simultaneous observations made with XMM–Newton and RXTE in 2002 and 2004. The X-ray spectra of both these extreme states exhibit strong reflection signatures, with a broad, skewed Fe Kα line clearly visible above the continuum. Using a newly developed, self-consistent reflection model which implicitly includes the blackbody radiation of the disc as well as the effect of Comptonization, blurred with a relativistic line function, we were able to infer the spin parameter of GX 339−4 to be 0.935 ± 0.01 (statistical) ±0.01 (systematic) at 90 per cent confidence. We find that both states are consistent with an ionized thin accretion disc extending to the innermost stable circular orbit around the rapidly spinning black hole." @default.
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- W2135893120 date "2008-07-11" @default.
- W2135893120 modified "2023-09-29" @default.
- W2135893120 title "A systematic look at the very high and lowhard state of GX3394: constraining the black hole spin with a new reflection model" @default.
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- W2135893120 doi "https://doi.org/10.1111/j.1365-2966.2008.13358.x" @default.
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