Up: B[e] stars
We have remarked that the lines of [Fe II] are weak and this characteristics
makes the object to stand out among the others studied in this series
where [Fe II] lines tend to be strong and numerous. The [Fe II]
weakness is only paralleled by HD 50138, where one also finds
numerous but weak [Fe II] lines.
Acknowledgements
It is an agreable task to thank Mr. Ph. Moreau
from the Haute Provence Observatory for the reproductions of the
spectra of Fig. 1.
Up: B[e] stars
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