**Table 1:** Spectroscopically confirmed Wolf-Rayet stars in IC 10 from catalogues of Massey et al. (1992), Royer et al. (2001) and Massey & Holmes (2002). Previous photometric and spectroscopic spectral types are taken from the above references, plus Massey & Armandroff (1995). Broad-band V and narrow-band v magnitudes are taken from archival WFPC2 imaging and Royer et al. (their c1), respectively, except those in parenthesis, which are obtained from GMOS spectrophotometry. See text for determination of absolute magnitudes. Line equivalent widths ( $W_{\lambda }$ ) and *FWHM* refer to He II $\lambda$ 4686 for WN stars, and C III $\lambda \lambda$ 4647-50/He II $\lambda$ 4686 plus C IV $\lambda \lambda$ 5801-12 for WC stars.
$\begin{table}\par\includegraphics[angle=90,clip]{tab1.eps}\par\end{table}$

Source LaTeX | All tables | In the text