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Fig. 41.
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G vs. GBP − GRP HRD showing the cross-match between the GALEX GR6+7 AIS catalogue with the GCNS (small symbols) and the candidate list of binaries with WD components with computed secondary star masses below the Chandrasekhar limit (< 1.4 ℳ⊙). The symbols are colour coded with the absolute FUV magnitude.
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