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Table 2.

Stellar parameters of the GJ1284 system and its two wide companions.

Parameter Value References (a)
Name and identifiers
Main identifier G 273-59 HD 221503 BD-17 6768
Gl 1284 898 897A 897B
TIC 9212046 434103018 434103039
Coordinates and kinematics
α (J2000) 23:30:13.44 23:32:49.40 23:32:46.98 23:32:46.98 2
δ (J2000) −20:23:27.46 −16:50:44.32 −16:45:12.34 −16:45:11.74 2
π [mas] 62.67 ± 0.09 68.70 ± 0.06 64.8 ± 4.1 (b) 2, 2, 3
d [pc] 15.906 ± 0.019 14.549 ± 0.006 15.15 ± 0.46 2, 2, 3
μα cos δ [mas a−1] 313.50 ± 0.15 340.98 ± 0.12 352.0 ± 2.6 2, 2, 3
μδ [mas a−1] −205.41 ± 0.15 −218.98 ± 0.07 −216.1 ± 2.7 2, 2, 3
Vr [km s−1] 0.84 ± 0.14 −0.845 ± 0.0012 −1.6 ± 1.7 1, 2, 4
U [km s−1] −13.837 ± 0.026 −13.942 ± 0.009 −15.4 ± 0.8 1
V [km s−1] −22.499 ± 0.021 −22.471 ± 0.007 −23.7 ± 0.7 1
W [km s−1] −10.231 ± 0.015 −9.184 ± 0.003 −9.1 ± 1.6 1
Spectral type and photometry
SpT M2–M2.5V + M3–M3.5V K6.0V M2.5V 1, 4, 5
B [mag] 12.59 ± 0.03 9.890 ± 0.019 11.79 ± 0.03 6, 7, 6
V [mag] 11.11 ± 0.03 8.600 ± 0.013 10.34 ± 0.04 6, 7, 6
G [mag] 9.9210 ± 0.0020 8.0816 ± 0.0008 10.033 ± 0.005 10.058 ± 0.004 2
BP [mag] 11.319 ± 0.003 8.829 ± 0.004 10.548 ± 0.008 10.556 ± 0.007 2
RP [mag] 8.777 ± 0.004 7.251 ± 0.004 8.198 ± 0.005 8.210 ± 0.009 2
J [mag] 7.200 ± 0.019 6.236 ± 0.019 6.71 ± 0.20 8
H [mag] 6.61 ± 0.04 5.61 ± 0.03 6.08 ± 0.03 8
K [mag] 6.329 ± 0.026 5.473 ± 0.016 5.858 ± 0.016 8
g [mag] 12.4084 ± 0.0010 10.86 ± 0.05 9.70 ± 0.04 9
r [mag] 10.50 ± 0.01 8.308 ± 0.011 9.91 ± 0.11 9
i [mag] 10.88 ± 0.05 9.72 ± 0.08 8.765 ± 0.021 9
NUV [mag] 18.02 ± 0.04 16.900 ± 0.015 17.253 ± 0.017 10, 11, 10
Additional information
v sin i [km s−1] 3.9 ± 1.2 7.47 ± 1.00 7.1 ± 1.2 12, 13, 4
pEW(Hα) [Å] −3.23 ± 0.08 0.12 ± 0.04 −1.051 12, 13, 14
log LX [erg s−1] (c) 29.04 ± 0.04 28.15 ± 0.11 29.22 ± 0.044 15
Prot [d] 7.45 ± 0.1 11.5 ± 0.1 5.00 ± 0.02 1

Notes.

(a)

Reference numbers for the three systems are separated by commas; a single number is provided whenever it is the same for all of them.

(b)

For the purposes of this work we adopt the parallax value from GJ 898 given the high uncertainty on the parallax determination of GJ 897 and their proximity and shared kinematics.

(c)

Calculated using the relations from Riaz et al. (2006).

References. (1) This work; (2) Gaia eDR3: Gaia Collaboration (2016, 2021); (3) Tokovinin (2018); (4) Torres et al. (2006); (5) Riaz et al. (2006) ; (6) APASS: Henden et al. (2016); (7) SKY2000: Myers et al. (2015); (8) 2MASS: Skrutskie et al. (2006); (9) UCAC4: Zacharias et al. (2013); (10) Schneider et al. (2019); (11) Riedel et al. (2017); (12) Jeffers et al. (2018); (13) López-Santiago et al. (2010); (14) Jones & West (2016); (15) ROSAT: Voges et al. (1999).

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