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Paper: |
Difference Frequencies of Non-radial Pulsation Modes and Repetitive Outbursts in Classical Be Stars |
Volume: |
508, The B[e] Phenomenom: Forty Years of Studies |
Page: |
93 |
Authors: |
Baade, D.; Rivinius, T.; Pigulski, A.; Carciofi, A.; BEST |
Abstract: |
Space photometry has revealed rich pulsation spectra in classical Be stars. Often frequency pairs can be found that differ by nearly the frequency of a third genuine stellar variability. The lowest currently known of these so-called difference (or Δ) frequencies reach 0.03 c/d, which is the upper limit of outburst frequencies. The potential of such slow variations for pulsation-assisted mass loss is discussed. |
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