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Table 10.

E(BV) in IC 10 fromseveral works, including this study.

Area E(BV) Method Reference
mag
Planetary nebulae 0.47 Planetary nebulae Ciardullo et al. (1989)
IC 10 0.75 – 0.80 WR stars Massey & Armandroff (1995)
IC 10 1.16 Cepheids Sakai et al. (1999)
IC 10 1.05 ± 0.10 Red supergiants Borissova et al. (2000)
IC 10 0.77 ± 0.07 Optical spectroscopy Richer et al. (2001)
IC 10 TRGB Hunter (2001)
IC 10 0.98 ± 0.06 UBV photometry Kim et al. (2009)
M#1 1.82 Brγ/Hα Borissova et al. (2000)a
1.57 Cloudy Hα This study
M#2 1.88 Brγ/Hα Borissova et al. (2000)a
1.72 Cloudy Hα This study
M#3 2.18 – 1.45 Brγ/Hα Borissova et al. (2000)a
2.01 Cloudy Hα This study
2.01 ± 0.06 Hα/Huα This study
A1#1 1.72 Brγ/Hα Borissova et al. (2000)a
1.73 Cloudy Hα This study
1.91 ± 0.05 Hα/Huα This study
A1#2 1.81 Brγ/Hα Borissova et al. (2000)a
1.85 Cloudy Hα This study
2.03 ± 0.03 Hα/Huα This study

Notes. (a) The error estimated is 10–15% and the clump M#3 is resolved in two H II regions.

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