New Mn II energy levels from the STIS-HST spectrum of the HgMn star HD 175640

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Volume 580 (August 2015)

A&A, 580 (2015) A10

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Table 4

Multiplet 3d⁵(⁶S)4d e⁷D−3d⁵(⁶S)4f e⁷F^o.

λ(CKC)^a	El(KS)^b	Eu(CKC)^a	Jl, Ju	Eu(KS)^b	λ(KS)^b
Å	cm^-1	cm^-1		cm^-1	Å

5294.276	79 540.93	98 424.00	1, 0	−	−
5294.296	79 540.93	98 423.93	1, 1	−	−
5294.318	79 540.93	98 423.858	1, 2	98 423.63	5294.379

5295.356	79 544.71	98 423.93	2, 1
5295.376	79 544.71	98 423.858	2, 2	98 423.63	5295.439
5295.400	79 544.71	98 423.773	2, 3	98 423.63	5295.439

5297.003	79 550.50	98 423.858	3, 2	98 423.63	5297.063
5297.024	79 550.50	98 423.773	3, 3	98 423.63	5297.063
5297.068	79 550.50	98 423.624	3, 4	98 423.60	5297.072

5299.288	79 558.56	98 423.773	4, 3	98 423.63	5299.327
5299.329	79 558.56	98 423.624	4, 4	98 423.60	5299.336
5299.387	79 558.56	98 423.424	4, 5	98 423.59	5299.338

5302.327	79 569.22	98 423.624	5, 4	98 423.60	5302.331
5302.382	79 569.22	98 423.424	5, 5	98 423.59	5302.333
5302.421	79 569.22	98 423.281	5, 6	98 423.56	5302.342

Notes. The energies and wavelengths from this paper are compared with those from Kramida & Sansonetti (2013). We note that with the new levels, all 15 of the possible lines of the ⁷D − ⁷F multiplet are known.

^(a)

CKC: this paper;

^(b)

KS: Kramida & Sansonetti (2013).

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