Oxygen-rich dust production in IC 10 | Astronomy & Astrophysics (A&A)

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Fig. 5

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V vs. B − V colors of stars toward IC 10 (Massey et al. 2007). Red points represent the candidate silicate-emission sources from this study. Small black points indicate LGGS sources within the search radius of the candidate silicate-emission sources (Table A.1).

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