Trumpler 16 in the CCCP (Wolk+, 2011)

Computer Science

Scientific paper

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Associations: Stellar, X-Ray Sources, Photometry: Infrared

Scientific paper

The bulk of the X-ray data discussed here were taken prior to the CCCP, as part of a guaranteed time program (2006 August 31, PI: S. Murray, 88.4 ks, ObsID 6402). A comprehensive analysis of those data was provided by Albacete-Colombo et al. 2008 (AC08, Cat. J/A+A/490/1055).
In this study, we limit our attention to the Trumpler 16 cluster and supplement the AC08 data with additional observations that partially overlap Tr 16 (ObsIDs 9482, 9483, 9488, in 2008 Aug-Sep and 6578 in 2006 Apr, and 4495 in 2004 Sep), which are described and mapped by Townsley et al. (2011ApJS..194....1T). We also invoke the new HAWK-I infrared observations (Preibisch et al. 2011, Cat. J/ApJS/194/10) for improved near-infrared counterpart information.
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