Stellar laboratories - IX. New Se v, Sr iv–vii, Te vi, and I vi oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191−B2B and RE 0503−289

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Table A.19

Calculated HFR oscillator strengths (log g_if_ik) and transition probabilities (g_kA_ki) in Sr vii.

	Lower level			Upper level


Wavelength^a/Å	energy^b/cm^-1	parity	J	energy^b/cm^-1	parity	J	log g_if_ik	g_kA_ki/s^-1	CF

Notes. CF is the absolute value of the cancellation factor as defined by Cowan (1981). In Cols. 3 and 6, e represents even and o odd.

^(a)

All wavelengths (given in vacuum for λ< 2000 Å, air for 2000 Å ≤ λ ≤ 20 000 Å, vacuum for 20 000 Å <λ) are deduced from experimental energy levels.

^(b)

Experimental energy levels taken from Sansonetti (2012).

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