Table 3
Observed values from three areas.
Ion | λobs (v) | F | I obs | N e |
(Å) (km s-1) | (mÅ) | (cm-3) | ||
|
||||
No. 6 – K | ||||
Fe xiv (rest) | 264.787 | 40 | 1660 | |
Fe xiv (bw) | 264.730 (57) | 45 | 542 | |
Fe xiv (rest) | 274.203 | 40 | 1310 | |
Fe xiv (dbl) | 1255 | 6 × 109 | ||
Fe xiv (bw) | 274.144 (65) | 48 | 230 | 1 × 1010 |
Fe xvi (rest) | 262.984 | 40 | 971 | |
Fe xvi (bw) | 262.926 (66) | 68 | 703 | |
Fe xvi (rest) | 262.984 | 40 | 1070 | |
Fe xvi (bw1) | 262.929 (63) | 45 | 497 | |
Fe xvi (bw2) | 262.837 (168) | 45 | 109 | |
|
||||
No. 8 – LT | ||||
Fe xiv (rest) | 264.787 | 40 | 1.15 × 103 | |
Fe xiv (bw) | 264.681 | 32 | 10 | |
Fe xiv (rest) | 274.204 | 42 | 1.15 × 103 | |
Fe xiv (dbl) | 1.14 × 103 | 2 × 109 | ||
Fe xiv (bw) | 274.080 | 30 | 6 | |
Fe xv (rest) | 284.160 | 45 | 8.3 × 103 | |
Fe xv (bw) | 284.081 | 60 | 270 | |
Fe xvi (rest) | 262.984 | 40 | 1.1 × 103 | |
Fe xvi (bw) | 262.908 | 34 | 54 | |
Fe xxiii | 263.758 | 70 | 304 | |
|
||||
No. 8 – K1 | ||||
Fe xiv (rest) | 264.787 | 40 | 2.7 × 103 | |
Fe xiv (bw) | 264.751 (41) | 42 | 1.6 × 103 | |
Fe xiv (rest) | 274.204 | 42 | 1.7 × 103 | |
Fe xiv (dbl) | 1.6 × 103 | 9 × 109 | ||
Fe xiv (bw) | 274.160 (47) | 43 | 5.2 × 103 | >1011 |
Fe xv (rest) | 284.160 | 45 | 1.26 × 104 | |
Fe xv (bw) | 284.110 (53) | 40 | 4.3 × 103 | |
Fe xvi (rest) | 262.985 | 40 | 2.1 × 103 | |
Fe xvi (bw) | 262.930 (62) | 50 | 1.3 × 103 | |
Fe xxiii | 263.722 (49) | 90 | 190 |
Notes. Observed wavelengths (λobs) are shown for the centroid position of the rest and blue-wing (bw) components. Values in parentheses are the corresponding velocities of the bw components towards the observer, in km s-1. The full-width-half-maximum (F) of the Gaussian line profile is then shown, together with the measured intensity Iobs (erg cm-2 s-1 sr-1), and the derived electron densities Ne from the Fe xiv line ratios. Rest wavelengths (Å) are 264.787, 274.203 (Fe xiv), 284.160 (Fe xv), 262.984 (Fe xvi), 263.765 (Fe xxiii). The intensity for the deblended Fe xiv (dbl) line is given.
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