... rotation

Figures 12 to 74 are only available in electronic form at http://www.edpsciences.org

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... community

http://www.astro.physik.uni-potsdam.de/PoWR.html

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... stars

Actually one star less, as we believe that WR 109 (classified in the WR catalog as WN5h+?) is erroneously counted here as a WN star. The typical brightness of a WN star would imply an implausible large distance ($D\!M$ = 17.4 mag), placing it beyond our Galaxy. From the binary period and the optical flickering, it has been concluded already (Steiner et al. 1988, 1999; Steiner & Diaz 1998) that WR 109 is a cataclysmic variable (CV).

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