Abstract
Within the framework of an optical and infrared spectrophotometric monitoring on a sample of PMS stars, we present some preliminary results on the behaviour of the Herbig Be star Z CMa.
A strong variability in H and Fe II line profiles is detected. The optical spectroscopic changes are connected with IR brightness variations.
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© 1988 D. Reidel Publishing Company
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Covino, E., Terranegra, L., Vittone, A., Giovannelli, F., Rossi, C. (1988). Fe II Line Profiles Variability in the Herbig Be Star Z CMa. In: Viotti, R., Vittone, A., Friedjung, M. (eds) Physics of Formation of FeII Lines Outside LTE. Astrophysics and Space Science Library, vol 138. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4023-9_17
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DOI: https://doi.org/10.1007/978-94-009-4023-9_17
Publisher Name: Springer, Dordrecht
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