Open Access
Table 1
Stellar and wind parameters roadmap.
| Property | Source | Assumed value |
|---|---|---|
| Spectral type | Literature (Table 2), MUSE spectrum(1) | |
| T* | tlusty fits of FLAMES spectrum(3), PoWR grid fit to MUSE spectrum(2) | |
| log g | tlusty fits of FLAMES spectrum(3), PoWR grid fit to MUSE spectrum(2) | |
| log L | SED fitting to UV spectrum(1) | |
| E(B−V) | SED fitting to UV spectrum(1) | |
| v sin i | Literature(3), Fourier transform fitting of He i λ 4921 & λ 6678 with iacob broad(1) | |
 |
PoWR fitting to UV spectrum(1) | |
| β | PoWR fitting to UV spectrum(1) | 0.8 |
| D | PoWR fitting to UV spectrum(1) | 10 |
| v∞ | PoWR fitting to UV spectrum(1) | From vesc |
| ξ (hydrostatic equation) | 10 km s−1 | |
| ξ(r) (emergent spectrum) | max(ξmin, 0.1 · v(r)), ξmin from spectral type/luminosity class (Table 4) |
Notes. Where no wind profile can be fit at this resolution within the UV data, the assumed values are listed.
References. (1) This work; (2) Rickard et al. (in prep.); (3) Dufton et al. (2019).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.