Reading between the lines - Disk emission, wind, and accretion during the Z CMa NW outburst

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Volume 643 (November 2020)

A&A, 643 (2020) A29

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Table 4

Lines that share a common upper level, among those with disk-like profiles.

Species	λ₀	A_ji	Uncertainty	Notes
	(Å)	(s⁻¹)
FeI	4786.8, 5262.9	1.03E+06, 8.70E+04	50%	Second one blended/uncertain
FeI	4839.5, 7511.0	3.90E+05, 1.35E+07	18%	Uncertain continuum (7511), blends
FeI	4939.7:, 5051.6, 5142.9	1.39E+04, 4.65E+04, 2.40E+04	40%	Blends
FeI	4957.6, 6271.3	4.22E+07, 3.05E+04	18%	Blends
FeI	5141.7, 6270.2	4.86E+05, 1.39E+05	50%	Blends
FeI	5393.2, 5615.6, 5709.4	4.91E+06, 2.64E+07, 2.13E+06	18%	Blends
FeI	5543.9, 5641.4	3.40E+06, 3.00E+06	50%	Strength too similar, uncertain
FeI	5572.8, 5624.5, 6408.0	2.28E+07, 7.41E+06, 3.12E+06	10%	OK first two lines
FeI	5747.9, 6103.3	8.80E+05, 1.52E+06	50%	Blends, uncertain
FeI	6191.6, 6256.4	7.41E+05, 7.40E+04	25%	OK
FeI	6393.6, 6462.7	4.81E+05, 9.70E+04	25%	OK
FeI	6265.1, 6335.3	6.84E+04, 1.58E+05	18%	Blends
FeI	6750.2, 8674.7, 8838.4	1.17E+05, 6.17E+05, 3.83E+05	25%	Strength too similar, uncertain

Notes. Uncertainty levels are taken from the NIST database and reflect the uncertainty in the atomic parameters for the most uncertain line. For lines with errors >40%, the theoretical line ratio is very uncertain, especially in cases in which the transition probabilities are not very different.

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