EDP Sciences
Free Access
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

Table A.1

LGGS sources within d < 4″ of the silicate emission candidates identified as members of IC 10.

Table A.2

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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