Table 10: Effective collision strengths at $3.0\times 10^5$ K for transitions from the ${\rm 1s}^2{\rm 2s}~^2{\rm S}_{1/2}$ ground level to the K-vacancy levels of Fe XXIV showing the effects of radiation and Auger dampings. ND: computed without damping. RD: radiation damping is included. R+AD: radiation and Auger dampings are included. Note: $a\pm b\equiv a\times 10^{\pm b}$ .
i k ND RD R+AD

1 4 2.96-3 1.19-3 1.11-3

1 5 1.26-3 5.43-4 5.05-4

1 6 2.23-3 1.55-3 1.19-3

1 9 3.19-3 2.94-3 2.92-3

1 10 3.28-5 1.60-5 1.49-5

1 13 6.36-5 4.37-6 2.05-6

1 14 1.70-5 6.41-6 2.61-6

1 15 4.07-6 3.71-6 1.46-6

1 17 6.54-6 6.11-6 1.98-6

1 18 3.34-6 3.28-6 2.08-6

**Table 10:** Effective collision strengths at $3.0\times 10^5$ K for transitions from the ${\rm 1s}^2{\rm 2s}~^2{\rm S}_{1/2}$ ground level to the K-vacancy levels of Fe XXIV showing the effects of radiation and Auger dampings. ND: computed without damping. RD: radiation damping is included. R+AD: radiation and Auger dampings are included. Note: $a\pm b\equiv a\times 10^{\pm b}$ .
i	k	ND	RD	R+AD
1	4	2.96-3	1.19-3	1.11-3
1	5	1.26-3	5.43-4	5.05-4
1	6	2.23-3	1.55-3	1.19-3
1	9	3.19-3	2.94-3	2.92-3
1	10	3.28-5	1.60-5	1.49-5
1	13	6.36-5	4.37-6	2.05-6
1	14	1.70-5	6.41-6	2.61-6
1	15	4.07-6	3.71-6	1.46-6
1	17	6.54-6	6.11-6	1.98-6
1	18	3.34-6	3.28-6	2.08-6

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