Constraint on the Spin of the Black Hole in GX 339-4 from X-ray Continuum
碩士 === 國立中央大學 === 天文研究所 === 99 === We present our analysis result for constraining the spin of the stellar-mass black hole (BH) in the X-ray binary GX 339-4 by fitting its X-ray continuum spectra. Reis et al. (2008) determined its spin to be a*=0.935±0.01 by modeling the profile of Fe K α line. Howe...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2011
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| Online Access: | http://ndltd.ncl.edu.tw/handle/59021460994432995624 |