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Cited by
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This article has been cited by the following publications. This list is generated based on data provided by Crossref.
Rivinius, Th. Baade, D. Štefl, S. and Maintz, M. 2001. Evolution in circumstellar envelopes of Be stars: From disks to rings?. Astronomy & Astrophysics, Vol. 379, Issue. 1, p. 257.
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Smith, Myron A. 2001. Ultraviolet Spectrophotometry of Variable Early‐Type Be and B Stars Derived from High‐ResolutionIUEData. The Astrophysical Journal, Vol. 562, Issue. 2, p. 998.
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Rivinius, Th. Baade, D. Štefl, S. Townsend, R. H. D. Stahl, O. Wolf, B. and Kaufer, A. 2001. Stellar and circumstellar activity of the Be star $\mathsf{\mu}$ Centauri. Astronomy & Astrophysics, Vol. 369, Issue. 3, p. 1058.
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Maintz, M. Rivinius, Th. Baade, D. and Štefl, S. 2002. Astero-Oscillometry: Gauging Stars with Oscillations. International Astronomical Union Colloquium, Vol. 185, Issue. , p. 222.
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Rivinius, Th. Baade, D. and Štefl, S. 2003. Non-radially pulsating Be stars. Astronomy & Astrophysics, Vol. 411, Issue. 2, p. 229.
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Štefl, S. Baade, D. Rivinius, Th. Stahl, O. Budovičová, A. Kaufer, A. and Maintz, M. 2003. Stellar and circumstellar activity of the Be starωCMa. Astronomy & Astrophysics, Vol. 411, Issue. 2, p. 167.
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Non-radial Pulsation Modeling of ω (28) CMa
  • Volume 175
  • M. Maintz (a1), Th. Rivinius (a1), S. Tubbesing (a1), B. Wolf (a1), S. Štefl (a2) and D. Baade (a3)
  • DOI: https://doi.org/10.1017/S0252921100055925
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Non-radial Pulsation Modeling of ω (28) CMa
  • Volume 175
  • M. Maintz (a1), Th. Rivinius (a1), S. Tubbesing (a1), B. Wolf (a1), S. Štefl (a2) and D. Baade (a3)
  • DOI: https://doi.org/10.1017/S0252921100055925
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Non-radial Pulsation Modeling of ω (28) CMa
  • Volume 175
  • M. Maintz (a1), Th. Rivinius (a1), S. Tubbesing (a1), B. Wolf (a1), S. Štefl (a2) and D. Baade (a3)
  • DOI: https://doi.org/10.1017/S0252921100055925
Available formats Please select a format to save.
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