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VizieR Correlated Data

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
[---]
1LB 3229C III4647.42   0.072   90 7.22
2LB 3229C III4650.25  -0.149   83 7.37
3LB 3229C III4651.47  -0.625   80 7.82
4LB 3229C III4186.90   0.924   64 7.64
5LB 3229N II3995.00   0.225   84 8.67
6LB 3229N II4041.31   0.830   80 8.71
7LB 3229N II4043.53   0.714   46 8.46
8LB 3229N II4176.16   0.600   70 8.86
9LB 3229N II4236.98   0.567   63 8.83
10LB 3229N II4241.78   0.728  105 9.06
11LB 3229N II4447.03   0.238   85 8.98
12LB 3229N III4097.33  -0.066  187 8.09
13LB 3229N III4103.43  -0.377  243 8.86
14LB 3229N III4640.64   0.140  227 8.51
15LB 3229N III4634.14  -0.108  186 8.50
16LB 3229N III4195.762-0.018  109 8.74
17LB 3229N III4200.102 0.241   85 8.24
18LB 3229Ne II4219.76  -0.150   40 9.16
19LB 3229Ne II4409.29   0.680   35 8.30
20LB 3229Ne II4290.37   0.920e 58 8.50
21LB 3229Ne II4290.60   0.830c    
22LB 3229Mg II4481.13   0.568  114 8.21
23LB 3229Si IV4088.85   0.199  250 7.71
24LB 3229Si IV4116.10  -0.103  157 7.26
25LB 3229Si IV4654.14   1.486  155 7.32
26LB 3229Si IV4212.41   0.804   71 7.24
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