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Table 4.

Reported orbital parameters for confirmed and candidate symbiotic binary stars in Gaia DR3.

Star 2MASS Gaia DR3 e P Type eLit PLit Ref.
identifier [d] [d]
StHA 32 J04374563–0119118 3229441606998725888 0.12 ± 0.03 618.47 ± 10.60 SB1 612 [1]
IV Vir J14163429–2145500 6276714894852124032 0.03 ± 0.02 279.98 ± 1.13 SB1 0 281.6 ± 1.2 [2]
AG Dra J16014101+6648101 1642955252784454144 0.28 ± 0.03 502.77 ± 6.01 SB1 0 548.65 ± 0.97 [3]
Hen 3-1213 J16351508–5142274 5934206543151802752 0.17 ± 0.06 530.11 ± 3.76 SB1 0.183 ± 0.034 533 ± 2 [4]
YY Her J18143419+2059213 4528063078197198848 0.15 ± 0.03 607.73 ± 8.37 SB1 589.5 ± 0.3 (a) [5]
StHA 176 J20224225–2107546 6859282948915521664 0.07 ± 0.07 246.64 ± 1.43 SB1
LT Del J20355722+2011275 1817300516637652352 0.40 ± 0.10 462.81 ± 6.88 SB1 465.6 [6]

TYC 1371-69-1 J07573112+2017347 670455944074475008 0.01 ± 0.01 119.13 ± 0.06 SB1 0.024 ± 0.015 119.18 ± 0.07 [7]
GaSS 1-4 J11121548–3207193 5403474822973970816 0.06 ± 0.04 458.92 ± 4.25 SB1 235 (a) [8]
SkySyC 1-3 J15265734–7003104 5796098502440628864 0.08 ± 0.02 701.13 ± 3.81 SB1 482.78 (a, b) [9]
IGR J15293-5609 J15292939–5612133 5883707000513657216 0.09 ± 0.04 31.50 ± 0.03 SB1
GaSS 1-20 J16005485–1628325 6250366095129668992 0.09 ± 0.14 10.51 ± 0.00 SB1
SS 295 J17073816–0744485 4360702354583742080 0.17 ± 0.10 471.11 ± 13.94 SB1 471.00 (a, b) [10]
Gaia DR3 217... J21180196+5721343 2178988199495779456 0.28 ± 0.10 753.92 ± 26.14 SB1
Gaia DR3 533... J11240425–6013342 5339026227414066432 0.07 ± 0.12 17.15 ± 0.02 SB1

CGCS 5926 J23454464+6252511 2016034975622911360
Gaia DR3 553... J08070625–4308520 5533253788183484672

Notes. Confirmed symbiotic systems are presented in the top panel of the table. Candidate systems for symbiotic stars with orbital solution and non-linear or acceleration solutions are reported in the middle and bottom panel, respectively. The first three columns report the commonly used identifier as well as the identifiers in the 2MASS and Gaia DR3 catalog. The next three columns report the orbital parameter and type of solution, presented in the TBO catalog (Gaia Collaboration 2023a). The last three columns report the most recent values in the literature and their reference.

(a)

Period obtained from photometric variability.

(b)

Orbital origin of the photometric variability with this period was suggested by Merc et al. (2019a).

References. 1: Mürset & Schmid (1999), 2: Smith et al. (1997), 3: Fekel et al. (2000), 4: Fekel et al. (2015), 5: Mikołajewska et al. (2002), 6: Munari & Jurdana-Šepić (2002), 7: Tang et al. (2012), 8: Munari et al. (2021), 9: Pojmanski (2002), 10: Jayasinghe et al. (2020).

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