Long-term coherent variations in the WR system EZ CMa : The binary scenario revisited J/A+A/347/583 J/A+A/347/583 EZ CMa spectroscopy Long-term coherent variations in the WR system EZ CMa : The binary scenario revisited L N Georgiev G Koenigsberger M M Ivanov N St-Louis O Cardona Astron. Astrophys. 347 583 1999 1999A&A...347..583G J/A+AS/119/37 : EZ CMa UBV + VBLUW photometry (Duijsens+, 1996) Binaries, spectroscopic Spectroscopy binaries: spectroscopic stars: individual (HD 50896, EZ Cma, WR6) stars: variables: general stars: Wolf-Rayet The table contains the window averaged flux (WAF) in two windows located at the P Cyg absorption component of the NV 4604/4620 doublet and the kurtosis of the HeII 4540 and HeII 4686 lines of the star EZ CMa. The three data sets are stored in three different files with the same format.
EZ CMaHD 50896WR 606 54 13.0-23 55 42
 WAF and Kurtosis for the SIT data WAF and Kurtosis for the SPM data WAF and Kurtosis for the Rozhen data JD Julian Date d WAV4604 Window averaged flux for the 4604{AA} window number=1 The units are arbitrary, because the spectra are normalized to the continuum. --- WAV4620 Window averaged flux for the 4620{AA} window number=1 The units are arbitrary, because the spectra are normalized to the continuum. --- KUR4686 Kurtosis for HeII 4686A line number=1 The units are arbitrary, because the spectra are normalized to the continuum. --- KUR4540 Kurtosis for HeII 4540A line number=1 The units are arbitrary, because the spectra are normalized to the continuum. --- Patricia Bauer CDS 1999Jun17Leonid Georgiev <georgiev@astroscu.unam.mx> J_A+A_347_583.xml