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HR 4074: an emission-free NRP twin of the Be star 28 CMa

  1. 1.
    0125051 - ASU-R 20020149 RIV US eng C - Conference Paper (international conference)
    Štefl, Stanislav - Rivinius, Th. - Baade, D.
    HR 4074: an emission-free NRP twin of the Be star 28 CMa.
    Radial and nonradial pulsations as probes of stellar physics. San Francisco: Astronomical Society of the Pacific, 2002, s. 248-249. ASP Conference Series., 259.
    [Colloquium of the International Astronomical Union /185./. Leuven (BE), 26.07.2001-31.07.2001]
    R&D Projects: GA AV ČR IAA3003001
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : Be stars * variables stars * line profiles
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    Echelle spectra obtained in 1999-2000 confirm that the southern B2IVe star HR 4074 shows conspicuous periodic line profile variations very similar to those known from proto-typical line profile-variable Be star 28(omega) CMa.
    Permanent Link: http://hdl.handle.net/11104/0023309
     

Number of the records: 1  

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