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- W1622499145 abstract "Abstract An alternative explanation to the light variations of some Be stars observed during their Be ⇌ Be-shell phase changes is proposed in terms of orbiting or passing clouds. Discrete ejections of matter and/or the presence of orbiting clouds suggest that the circumstellar envelopes of these Be stars may be clumpy." @default.
- W1622499145 created "2016-06-24" @default.
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- W1622499145 date "2000-01-01" @default.
- W1622499145 modified "2023-09-24" @default.
- W1622499145 title "Light Curves of Be Stairs due to Orbiting Arcs of Matter or Prominence-Like Structures" @default.
- W1622499145 cites W2006415601 @default.
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- W1622499145 doi "https://doi.org/10.1017/s0252921100056086" @default.
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