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Table 3
Linear fit coefficients of flux-flux relationships for the M dwarfs from MA11.
| Line 1 | Line 2 | N∗ | c1 | c2 |
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| Ca K | Ca H | 24 | 0.82 ± 0.46 | 0.86 ± 0.08 |
| Hα | Ca K | 22 | −1.32 ± 0.85 | 1.26 ± 0.15 |
| X-rays | Hα | 18 | −1.02 ± 0.94 | 1.29 ± 0.15 |
| Hα | Hβ | 16 | −0.66 ± 0.41 | 1.03 ± 0.07 |
| Hα | Hγ | 14 | −1.33 ± 0.32 | 1.06 ± 0.05 |
| Hα | Hδ | 13 | − 2.36 ± 0.47 | 1.20 ± 0.08 |
| Hα | Hϵ | 10 | −14.66 ± 5.63 | 2.96 ± 0.87 |
| Hβ | Hγ | 14 | −0.94 ± 0.18 | 1.08 ± 0.03 |
| Hβ | Hδ | 13 | −1.40 ± 0.14 | 1.14 ± 0.03 |
Notes. Linear regression fits are of the type log F1 = c1 + c2 × log F2 and Col. 3 gives the number of stars in the sample.
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