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.
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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