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Table 2:

Relative intensities of prominent emission lines of V838 Her on 1991 April 2.

$\lambda_{\rm obs}$
Int. ident.
(Å)    
3966 26.0: H$\epsilon$, [Ne III] 3967.5
4051 1.0 C III 24, 4056.1
4101 36.2 H$\delta$
4206 0.8 C IV 11, 4217
4248 2.8 C II 6, 4267.0, 4267.3
4341 47.5 H$\gamma$
4467 5.9 He I 4471
4611 2.9 N II 5, 4607.2, 4613.9
4647 7.5 N III 2, 4640.6, 4641.9, C III 1, 4650.2
4688 4.3 He II 4686
4724 1.2: He I 4713, [Ne IV] 4720
4861 100 H$\beta$
4934 1.9: He 1 4922, Fe II 4924
5027 7.2 C IV 3, 5021,5023, He I 5016, Fe II 5018
5076 1.1: Si II 5, 5056?
5167 2.1 Fe II 42, 5169.0
5314 0.7 Fe II 49, 5316.6
5468 0.8 N II 2, 5462.6
5675 3.5 N II 3, 5679.6, C III 2, 5696.0
5796 1.4: C IV 1, 5801.5, 5812.1
5872 20.2 He I 5876, C III 20, 5871.6, 5894.1
6129 0.7 C III 13, 6154.4, 6156.6
6268 0.2 blue peak of [S III] 6310
6353 6.2 Si II 2, 6341, 6371 [S III] 6310
6559 435 H$\alpha $
6672 5.0: He I 6678
7060 13.2: He I 7065, C II 20, 7115

Notes. The effect of the interstellar extinction is corrected by E(B-V)=0.53.


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