摘要：In our paper Barniske et al. (2008), we erroneously as-
signed the K-band magnitude K = 9.93mag of the source
2MASS17461090-2849074 from the 2MASS All-Sky Catalog
of Point Sources (Cutri et al. 2003) to the nearby Wolf-Rayet
type star WR102c. This resulted in an overestimate of the stel-
lar bolometricluminosityof WR102c.The correct K-bandmag-
nitude of WR102c is K = 11.6mag (Figer et al. 1999). A
comprehensive spectroscopic analysis of WR102c is provided
by Steinke et al. (2016), where the correct K-band magnitude
is used. The newly derived bolometric luminosity of WR102c
is logL/L ? = 5.5...5.7 and the ionizing photon flux [s −1 ] is
log(Φ Ly ) = 49.0...49.3.
