The rotation rates of massive stars - How slow are the slow ones?

J. O. Sundqvist; S. Simón-Díaz; J. Puls; N. Markova

doi:10.1051/0004-6361/201322761

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Volume 559 (November 2013)

A&A, 559 (2013) L10

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Fig. 3

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Same as Figs. 1 and 2, but now with the observed O III line artificially symmetrized about line-center. We note the overlap of the blue and red squares in the middle panel, indicating perfect agreement between vsini derived from the FT and GOF methods.

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