Abstract
We present here the Hα spectra of 44 Be stars taken at a resolution of 0.5 Å. From the spectra, different emission line parameters have been deduced. A study of the correlations between different pairs of these parameters has been made with a view to understanding the mechanisms of line formation and shaping in Be stars.
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APA
Banerjee, D. P. K., Rawat, S. D., & Janardhan, P. (2000). Hα observations of Be stars. Astronomy and Astrophysics Supplement Series, 147(2), 229–242. https://doi.org/10.1051/aas:2000299
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