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Stellar and wind parameters obtained from line profile fits of observations taken in Arizona in 2013.
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Fig. 3
Sequence of fits to daily line variations of H and He lines in 2013. Fits to the different line transitions are achieved using individual values of νmic and νmac (for details see Sect. 4.1). |
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Fig. 3
continued. |
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Fig. 3
continued. |
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Fig. 4
Hα line profiles taken in 2009 and 2010 at Ondřejov Observatory together with their corresponding model fits (for details see Table 2). Lines with highly complex profiles or roughly zero EW have not been fitted. |
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Fig. 5
Same as Fig. 4, but for data taken in 2011. |
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Fig. 6
Same as Fig. 4, but for data taken in 2012 (top) and 2013 (bottom). |
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Fig. 7
Fits to the lines of Si ii λλ 4128, 4130 Å, and Si iii λ 4552 Å in the Arizona spectra. Fits to the different line transitions are achieved using individual values of νmic and νmac (for details see Sect. 4.1). |
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© ESO, 2015