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Issue A&A
Volume 504, Number 1, September II 2009
Page(s) 211 - 211
Section Stellar structure and evolution
DOI http://dx.doi.org/10.1051/0004-6361/20078511e
Published online 11 August 2009

A&A 504, 211-211 (2009)
DOI: 10.1051/0004-6361/20078511e

Erratum

The VLT-FLAMES survey of massive stars: atmospheric parameters and rotational velocity distributions for B-type stars in the Magellanic Clouds

I. Hunter1, D. J. Lennon2, P. L. Dufton1, C. Trundle1, S. Simón-Díaz3, S. J. Smartt1, R. S. I. Ryans1, and C. J. Evans4

1  Astrophysics Research Centre, School of Mathematics & Physics, The Queen's University of Belfast, Belfast, BT7 1NN, Northern Ireland, UK
2  Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
3  LUTH, Observatoire de Meudon, 5 Place Jules Janssen, 92195 Meudon Cedex, France
4  UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK

A&A 457, 265–280 (2006), DOI: 10.1051/0004-6361:20065392 A&A 479, 541–555 (2008), DOI: 10.1051/0004-6361:20078511

Abstract
We correct the estimates of the dispersions in the rotational velocities for early-type stars in our Galaxy (Dufton et al. 2006, A&A, 457, 265) and the Magellanic Clouds (Hunter et al. 2008, A&A, 479, 541). The corrected values are $\pi^{\frac{1}{4}}$  (i.e. approximately 33%) larger than those published in the original papers.


Key words: stars: early-type -- stars: fundamental parameters -- stars: rotation -- stars: evolution -- errata, addenda



© ESO 2009

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