| Issue |
A&A
Volume 546, October 2012
|
|
|---|---|---|
| Article Number | A94 | |
| Number of page(s) | 13 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/201220087 | |
| Published online | 11 October 2012 | |
Online material
Appendix A: Cross-correlation LGGS stars – silicate emission candidates
LGGS sources within d < 4″ of the silicate emission candidates identified as members of IC 10.
LGGS sources within d < 4″ of the silicate emission candidates identified as field stars.
The silicate emission candidates from Table 1 are matched with optical sources from the LGGS in Sect. 4.3. When several
LGGS stars fall within 4″ of the silicate emission source coordinates, we selected the closest LGGS star. We list in Tables A.2 and A.1 the LGGS sources within 4″ from each silicate emission candidate. We also list their optical colors. In all cases, the closest LGGs star is also the best match in terms of brightness and red color.
© ESO, 2012
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