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Tracing the transient periods in the Be star 28 .omega. CMa

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    0124695 - ASU-R 20000154 RIV US eng C - Conference Paper (international conference)
    Štefl, Stanislav - Budovičová, Andrea - Baade, D. - Kaufner, A. - Rivinius, T. - Stahl, O. - Wolf, B.
    Tracing the transient periods in the Be star 28 .omega. CMa.
    The Be phenomenon in early-type stars. San Francisco: Astronomical Society of the Pacific, 2000 - (Smith, M.; Henrichs, H.; Fabregat, J.), s. 240-243
    [Colloquium of the International Astronomical Union /175./. Alicante (ES), 28.06.1999-02.07.1999]
    Institutional research plan: CEZ:AV0Z1003909
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    Spectra of the Be star 28 CMa obtained with the HEROS echelle spectrograph were used to check the presence of transient periods in commonly measured scalar parameters of absorption and emission lines.
    Permanent Link: http://hdl.handle.net/11104/0022954
     

Number of the records: 1  

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