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Table 5.

Coronal lines in V745 Sco, V3890 Sgr and V407 Cyg spectra.

Event Dataset Line t[days] Line strength
V745 Sco 1989 CTIO [Fe X] 6374 Å 5 9.71 × 10−11
9 3.93 × 10−11
22 4.37 × 10−12
[Ar X] 5535 Å 5 8.42 × 10−11
9 2.51 × 10−11
22 2.70 × 10−12
317 1.77 × 10−13
V745 Sco 2014 SMARTS [Fe X] 6374 Å 3.5 1.11 × 10−11
6 1.12 × 10−11
[Fe XI] 7892 Å 3.5 6.39 × 10−12
6 6.29 × 10−12
[Fe XIV] 5303 Å 3.5 7.24 × 10−12
6 7.32 × 10−12
[Ar X] 5535 Å 3.5 3.65 × 10−12
6 3.53 × 10−12
V745 Sco 2014 SAAO [Fe X] 6374 Å 4.5 1.09 × 10−10
6 2.99 × 10−12
86 2.09 × 10−12
[Fe XIV] 5303 Å 86 9.24 × 10−13
[Ar X] 5535 Å 3 8.74 × 10−11
V3890 Sgr 1990 IUE low res. [Fe XI] 2648 Å 19 1.14 × 10−10
27 4.53 × 10−11

Notes. CTIO and Ondřejov data are binned and averaged over intervals of 3 days, SMARTS and SAAO of 2. Units are erg cm−2 s−1 for CTIO, SMARTS, SAAO and IUE, counts for Ondřejov.

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