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The Herbig Ae/Be Star V586 Ori
Authors:I. N. Chkhikvadze
Affiliation:(1) Abastumani Astrophysical Observatory, Georgia
Abstract:Studies of the Herbig Ae/Be star V586 Ori based on photoelectric observations in the Strömgren system are reported. It is found that as the brightness decreases, the Balmer discontinuity index initially increases and then begins to drop. As the star fades, the index beta decreases. We have previously found similar variations in the indices beta and C for UX Ori, RR Tau, and V351 Ori. It is shown that V586 Ori has the characteristics of a shell-star.
Keywords:stars photometry  individual stars  V586 Ori
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