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Table 1

Properties of the HK Tau system.

Entire system
Parameter Value References
Separation 2.34″, ~300 au (1)
Distance 128 ± 4 pc (2), (3)
Single components
Parameter A B References
Inclination 56.90.5+0.5Mathematical equation: $\[56.9_{~~-0.5}^{\circ+0.5}\]$ 83.20.2+0.2Mathematical equation: $\[83.2_{~~-0.2}^{\circ+0.2}\]$ (4)
Position angle 175° 41° (5), (6)
Stellar mass 0.440.11+0.14Mathematical equation: $\[0.44_{-0.11}^{+0.14}\]$ 0.370.2+0.2Mathematical equation: $\[0.37_{-0.2}^{+0.2}\]$ M (4)
Spectral type M1 M2 (7)
Stellar luminosity 0.550.15+0.15Mathematical equation: $\[0.55_{-0.15}^{+0.15}\]$ 0.030.01+0.01Mathematical equation: $\[0.03_{-0.01}^{+0.01}\]$ L (8)
Stellar radius × sin(i) 1.400.1+0.1Mathematical equation: $\[1.40_{-0.1}^{+0.1}\]$ R (9)
Systemic velocity 5.980.51+0.09Mathematical equation: $\[5.98_{-0.51}^{+0.09}\]$ 6.050.37+0.7Mathematical equation: $\[6.05_{-0.37}^{+0.7}\]$ km/s (10)

Notes. (1) White & Ghez (2001), (2) Gaia Collaboration (2021), (3) Luhman (2023); the distance is estimated from the primary, (4) Manara et al. (2019), (5) Leinert et al. (1993), (6) Villenave et al. (2020), (7) Monin et al. (1998), (8) Simon et al. (2019); the luminosity of B is likely underestimated because of its inclination, (9) Nofi et al. (2021), (10) Braun et al. (2021); the systemic velocity is measured from ALMA data in kinematic local standard of rest reference.

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