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Table 3

Orbital solutions of θ2 Tau A and B from various techniques.

Spectroscopic orbital solution (FDBinary)
Parameter This work

P (days) 140.728161
T 1993.0751
e 0.734662
ωB (°) 235.88
KA (km s-1) 32.74
KB (km s-1) 43.402 (± 0.5, cf. text)

Interferometric Orbital Solution (AM06)

P (days) 140.728161
T 1989.60701  ±  0.00003
e 0.73725  ±  0.00036
a (mas) 18.796  ±  0.056
i (°) 47.61  ±  0.09
Ω (°) 173.73  ±  0.07
ωA (°) 55.40  ±  0.06
πsec (mas) 22.303  ±  0.36

Astrometric-Spectroscopic Orbital Solution
Parameter This work TSL97

P (days) 140.7302  ±  0.0002 140.72816  ±  0.00093
T 1995.00144  ±  0.00002 1993.0752  ±  0.0008
e 0.7360  ±  0.0003 0.7266  ±  0.0049
a (mas) 18.91  ±  0.06 18.604  ±  0.20
i (°) 47.8  ±  0.1 46.24  ±  1.0
Ω (°) 353.82  ±  0.09 171.24  ±  1.8
ωB (°) 235.41  ±  0.08 236.4  ±  1.1
0.754  ±  0.001 0.873  ±  0.048
πorb (mas) 20.90  ±  0.10 21.22  ±  0.76
KA (km s-1) 32.95  ±  0.04 33.18  ±  0.49
KB (km s-1) 43.68  ±  0.14 385  ±  2
MA (M) 2.86  ±  0.03 2.42  ±  0.30
MB (M) 2.16  ±  0.02 2.11  ±  0.17
rss (all) 1.23e+3 8.18e+03
System mass (M) 5.02  ±  0.09 4.54  ±  0.51
Time span (yr) 20.0 6.3

Notes. The standard deviations including orbital parallax and masses are shown in the bottom panel.

(1)

Fixed (adopted from TSL97).

(2)

Fixed (see Sect. 3).

(3)

Adopted from de Bruijne et al. (2001) (not an orbital element).

(4)

Adopted from PS92.

(5)

Fixed (after a search in 2-D space).

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