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 | ![]() |
![]() |
(4) |
| Position angle | 175° | 41° | (5), (6) |
| Stellar mass | ![]() |
M⊙
|
(4) |
| Spectral type | M1 | M2 | (7) |
| Stellar luminosity | ![]() |
≥ L⊙
|
(8) |
| Stellar radius × sin(i) |
R⊙
|
− | (9) |
| Systemic velocity | ![]() |
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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