Table 7: Abundance ratios (relative to Asplund et al. 2005) applying temperature structure-independent linear combinations of coronal emission lines. Values given in brackets for EQ Peg A correspond to the quiescent state.

Ratio	EQ Peg A		EQ Peg B
O/N	0.83  0.20	(1.00  0.29)	0.81  0.72
Ne/O	2.48  0.31	(2.02  0.16)	2.18  0.41
Mg/Ne	0.20  0.02	(0.19  0.02)	0.32  0.07
Si/Mg	2.52  0.21	(2.56  0.25)	2.05  0.44
S/Si	1.26  0.20	-	-
Ne/Fe	7.30  0.64	(5.99 0.34)	5.45 0.78
Mg/Fe	1.27  0.17	(1.09 0.19)	1.63 0.43