Properties of WNh stars in the Small Magellanic Cloud: evidence for homogeneous evolution

F. Martins; D. J. Hillier; J. C. Bouret; E. Depagne; C. Foellmi; S. Marchenko; A. F. Moffat

doi:10.1051/0004-6361:200811014

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Volume 495 / No 1 (February III 2009)

A&A, 495 1 (2009) 257-270

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Table 1:

Photometry of the target stars from Massey & Duffy (2001) together with the derived extinction.
Star	ST	U	B	V	E(B-V)
					Gal.+ SMC
SMC-WR1	WN3h	14.22	15.13	15.17	0.24
SMC-WR2	WN5h	13.26	14.08	14.26	0.03+0.06
SMC-WR4	WN6h	12.48	13.25	13.37	0.04+0.10

Source LaTeX | All tables | In the text

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