Colloquium: Thomas Rivinius 3:15 pm
Colloquium: Thomas Rivinius
Feb 24 @ 3:15 pm – 4:15 pm
Our Current Understanding of Classical Be Stars Dr. Thomas Rivinius, Chile, ESO Paranal I will introduce Be stars as B-type stars with gaseous disks in Keplerian rotation. These disks form by mass ejection from the star itself...
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