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Home All issues Volume 515 (June 2010) A&A, 515 (2010) A47 Full HTML
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Table 3:

Intensities of the observed lines and of those simulated by Cloudy corresponding to the best-fit and normalized to the O VIII Ly-$\alpha $ flux (see text and Fig. 6 for more details).
Line ID $\lambda_{\rm exp} ({\rm {\AA}})$ Observed ratio Cloudy predicted ratio
Ne X Ly-$\alpha $   12.134  $0.2_{\rm -0.2}^{+0.2}$  0.2
Ne IX (r)   13.447  $\la$0.1  0.1
Ne IX (i)   13.550  $\la$0.1  0.2
Ne IX (f)   13.700  $ 0.7_{\rm - 0.2}^{+ 0.2}$  0.6
Fe XVII 3s-2p   17.073  $ 0.5_{\rm -0.2}^{+0.2}$  -
O VIII Ly-$\alpha $   18.969  $ 1.0_{\rm -0.2}^{+0.2}$  1.0
O VII (r)   21.600  $\la$0.1  0.3
O VII (i)   21.790  $ 1.0_{\rm -0.2}^{+0.2}$  0.6
O VII (f)   22.101  $ 2.2_{\rm -0.3}^{+0.3}$  2.5
N VII Ly-$\alpha $   24.781  $ 0.3_{\rm -0.1}^{+0.1}$  0.2
N VI (r)   28.787  $\la$0.13  0.01
N VI (i)   29.083  $ 0.1_{\rm - 0.1}^{+ 0.1}$  0.01
N VI (f)   29.534  $ 0.5_{\rm - 0.1}^{+ 0.1}$  0.1
C VI Ly-$\alpha $   33.736  $ 0.5_{\rm -0.2}^{+0.2}$  0.7


Source LaTeX | All tables | In the text

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