Table 1.
Orbital parameter and best spatiokinematic fit.
Orbital parameters | Parametric fit | ||
---|---|---|---|
Period [days] | 1279.4 ± 0.23 | i [°] | 69.88 |
Eccentricity | 0.22 ± 0.00 | θout [°] | 49.56 |
T0 [days] | 2456309 ± 112 | θin [°] | 49.31 |
ω [°] | 11 ± 73 | θcav [°] | 25.14 |
K1 [km s−1] | 13.264 ± 0.005 | ϕtilt [°] | −4.65 |
γ [km s−1] | 6.1 ± 0.1 | vin [km s−1] | 158 |
Semi-major axis (a) [R⊙] | 586 | vout [km s−1] | 37 |
Roche-lobe radius (RL) [R⊙] | 395 | cv | 0.04 |
pv | 2.32 | ||
pρ, in | 14.92 | ||
pρ, out | −9.89 | ||
cτ | 2.29 | ||
R1 [R⊙] | 105.4 | ||
R2 [R⊙] | 1.04 | ||
Rin [R2] | 8.6 | ||
Rout [RL] | 1.00 |
Notes. Listed in the table are all orbital parameters of the object HD 52961. Here, “Period” is the time of one revolution in days; “Eccentricity” defines the elongation of the orbit; T0 sets the position of the orbit at phase zero; ω is the argument of periapsis, which defines the orientation of the ellipse; K1 is the highest radial velocity offset from the median; γ is the radial velocity of the mass centre. The semi-major axis and the Roche-lobe radius was calculated assuming an inclination of 60°. The second column shows the best-fit parameters of HD 52961 found using the parametric fit described in Bollen et al. (2022). The tabulated parameters are: (i) inclination angle of the binary system; (θout) jet outer angle; (θin) jet inner angle; (θcav) jet cavity angle; (ϕtilt) jet tilt; (vin) inner jet velocity; (vout) jet velocity at the jet edges; (cv) velocity scaling parameter; (pv) exponent for the velocity profile; (pρ, in, pρ, out) exponent for the density profile for the outer and inner region; (cτ) optical depth scaling parameter; (R1) the radius of the post-AGB star. The term R2 is the radius of the secondary. Underneath the line, the inner and outer launching radius is shown.
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