Abstract
We present the spectroscopic variations of 14 program Be stars observed within 2008 - 2009 at the Bosscha Observatory, Lembang, Indonesia. The Be stars show spectroscopic profiles as Be and Be-shell, and sometimes as B-normal. These profiles come from the disk-like envelope or rings surrounded the star’s equatorial plane. Our program stars are: 5 as Be single-peaked, 2 as Be double-peak, and 7 as B-normal stars. We also measure the Ip/Ic ratio from the line profiles.
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