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Home All issues Volume 636 (April 2020) A&A, 636 (2020) A99 Full HTML
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Fig. A.1.

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Stellar wind mass loss rate as a function of luminosity of hydrogen depleted massive stars. Panel a: solid blue line: Brussels. Dashed red line: WNE Potsdam. Dotted gray line: WC Potsdam. Panel b: solid blue line: Brussels. Dashed red line: Tramper WC Y = 0.98. Dotted gray line: Tramper WC Y = 0.6. Panel c: dashed red line: Potsdam. Dotted gray line: Yoon fWR = 1. Panel d: solid blue line: Brussels. Dashed green line: Warsaw.

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