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Table 5.

Optical and X-ray properties of classified Galactic M dwarfs in the filed of the Draco dSph.

Src-No r − i i − z z − J Spectral type Mi dphot (pc) dGaia (pc) Mbol Lx (erg s−1) log
3 0.92±0.01 0.52±0.02 1.21±0.08 M2 8.8±0.1 506 8.6 8.5  ×  1028 –2.9
7 1.33±0.02 0.70±0.02 1.38±0.10 M4 9.34±0.3 520 366±23 9.5 3.2  ×  1029 –2.1
9 1.15±0.01 0.64±0.01 1.28±0.06 M3 8.8±0.3 413 497±20 8.2 1.4  ×  1029 –3.0
10 1.74±0.04 0.98±0.03 1.59±0.13 M5 11.7±0.4 242 657±160 9.1 2.5  ×  1029 –2.5
12 1.40±0.02 0.78±0.02 1.51±0.05 M4 10.0±0.3 351 446±28 8.7 2.0  ×  1029 –2.7
13 1.14±0.04 0.64±0.04 1.32±0.19 M3 9.2±0.5 820 9.7 3.0  ×  1029 –2.4
14 1.45±0.01 0.80±0.01 1.44±0.04 M4-M5 10.2±0.3 158 140±2 9.7 1.2  ×  1028 –3.3
15 1.15±0.01 0.62±0.01 1.37±0.06 M3 9.1±0.1 375 510±70 8.3 2.3  ×  1029 –2.8

Notes. The spectral types of the M dwarfs are identified based on the optical and infrared colours (West et al. 2011). The table also presents the absolute magnitude (Mi), bolometric magnitude (Mbol), photometric distance (dphot), Gaia DR2 distance (dGaia), X-ray luminosity (LX) in the energy range of 0.2–5.0 keV, and X-ray to bolometric luminosity, log, of M dwarfs.

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