Free Access
Volume 578, June 2015
Article Number A107
Number of page(s) 9
Section Stellar structure and evolution
Published online 12 June 2015

Online material

Appendix A: On the clumping factor and mass-loss rate dependency

thumbnail Fig. A.1

Observed spectrum (thin blue line) – H band (left panel), K band (right panel) – compared with the best-fitting PoWR model (dotted line) for different D factors: D = 10 (top panel); D = 4 (middle panel); D = 1 (low panel).

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© ESO, 2015

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