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How Strong is the Evidence of Superionization and Large Mass Outflows in B/Be Stars? 2. The C IV and SI IV Lines in the UV Spectra of V 767 Cen, ο And, Θ CrB, λ Eri, and 59 CYG

Harmanec, P.; Hubeny, I.; Stefl, S.

The theoretical spectra in the neighborhood of the C IV and Si IV resonance lines have been compared with the published observed spectra of five Be stars, V 767 Cen, omicron And, Theta CrB, Lambda Eri, and 59 Cyg. It is shown that the published determinations of large outflow velocities evidenced by a violet asymmetry of the C IV and Si IV lines, …