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Table 10.
E(B–V) in IC 10 fromseveral works, including this study.
Area | E(B–V) | 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 | |
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