The VLT-FLAMES Tarantula Survey - XI. A census of the hot luminous stars and their feedback in 30 Doradus

E. I. Doran; P. A. Crowther; A. de Koter; C. J. Evans; C. McEvoy; N. R. Walborn; N. Bastian; J. M. Bestenlehner; G. Gräfener; A. Herrero; K. Köhler; J. Maíz Apellániz; F. Najarro; J. Puls; H. Sana; F. R. N. Schneider; W. D. Taylor; J. Th. van Loon; J. S. Vink

doi:10.1051/0004-6361/201321824

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Volume 558 (October 2013)

A&A, 558 (2013) A134

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Fig. C.1

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Determination of R_V for 30 Dor. In the R136 region a): the M_V of single O-type stars derived from HST/WFC3 photometry is plotted against the expected M_V derived from VLT-MAD K-band photometry after applying the Martins & Plez (2006) calibration. In the MEDUSA region b): the M_V derived from VFTS photometry is plotted against the expected M_V derived from IRSF K-band photometry after applying the Martins & Plez (2006) calibration. Solid lines indicate the 1:1 relations.

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