VizieR

J/MNRAS/409/582/tablea1

Helium-rich subluminous B stars abundances (Naslim+, 2010)

Oscillator strength, measured equivalent width and derived elemental abundance for each line measured in the six programme stars (254 rows)

Full	Name	Ion	lambda 0.1nm	n_	loggf [-]	n_	EW 0.1nm	eps [---]
1	LB 3229	C III	4647.42		0.072		90	7.22
2	LB 3229	C III	4650.25		-0.149		83	7.37
3	LB 3229	C III	4651.47		-0.625		80	7.82
4	LB 3229	C III	4186.90		0.924		64	7.64
5	LB 3229	N II	3995.00		0.225		84	8.67
6	LB 3229	N II	4041.31		0.830		80	8.71
7	LB 3229	N II	4043.53		0.714		46	8.46
8	LB 3229	N II	4176.16		0.600		70	8.86
9	LB 3229	N II	4236.98		0.567		63	8.83
10	LB 3229	N II	4241.78		0.728		105	9.06
11	LB 3229	N II	4447.03		0.238		85	8.98
12	LB 3229	N III	4097.33		-0.066		187	8.09
13	LB 3229	N III	4103.43		-0.377		243	8.86
14	LB 3229	N III	4640.64		0.140		227	8.51
15	LB 3229	N III	4634.14		-0.108		186	8.50
16	LB 3229	N III	4195.76	2	-0.018		109	8.74
17	LB 3229	N III	4200.10	2	0.241		85	8.24
18	LB 3229	Ne II	4219.76		-0.150		40	9.16
19	LB 3229	Ne II	4409.29		0.680		35	8.30
20	LB 3229	Ne II	4290.37		0.920	e	58	8.50
21	LB 3229	Ne II	4290.60		0.830	c
22	LB 3229	Mg II	4481.13		0.568		114	8.21
23	LB 3229	Si IV	4088.85		0.199		250	7.71
24	LB 3229	Si IV	4116.10		-0.103		157	7.26
25	LB 3229	Si IV	4654.14		1.486		155	7.32
26	LB 3229	Si IV	4212.41		0.804		71	7.24

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