Table A.2.
Orbital and mass-related parameters of non-eclipsing HBSs discussed here.
| Star | Porb | a sin i or | e | ω | T0 [HJD − | M1sin3i | M2sin3i | SB | Ref. |
|---|---|---|---|---|---|---|---|---|---|
| [d] | a1 sin i [R⊙] (a) | [°] | 2 400 000] | or f(M) [M⊙] (a) | |||||
| HD 24623 | 19.663042(14) | 43.78(3) | 0.48873(38) | 130.18(6) | 52934.5350(25) | 1.4692(26) | 1.4423(27) | SB2 | (1) |
| HD 87810 | 12.94724(12) | 25.57(8) | 0.439(2) | 48.6(3) | 47442.274(8) | 0.670(6) | 0.668(6) | SB2 | (2) |
| ET UMa | 11.57907(19) | 22.9(6) | 0.26(4) | 171.0(16) | 18468.18(6) | 0.75(5) | 0.45(3) | SB2 | (3) |
| p Vel A | 10.210406(15) | 16.0(4) | 0.508(12) | 185.0(15) | 16461.18(4) | 0.287(20) | 0.243(12) | SB2 | (4) |
| θ Car | 2.20288(1) | 0.8174(22) | 0.129(2) | 81.8(17) | 54302.898(9) | 0.001510(12) | SB1 | (5) | |
| θ1 Cru | 24.4828 | 39.2(10) | 0.609(8) | 358.9(14) | 19453.35(5) | 0.74(6) | 0.61(4) | SB2 | (6) |
| ζ Cen | 8.02352 | 37.1(25) | 0.5 (b) | 290 (b) | 29798.46 | 6.3(7) | 4.4(7) | SB2 | (7) |
| HD 126983 | 11.8(4) | 33(4) | 0.33(15) | 42(7) | 41440.4(26) | 1.72(27) | 1.59(27) | SB2 | (8) |
| HD 158013 | 8.2159 | 5.20(7) | 0.333(9) | 132.1(21) | 31979.003(49) | 0.0279(9) | SB1 | (9) | |
| HD 181470 | 10.3932 | 25.3(10) | 0.520(19) | 199(3) | 23570.62(5) | 1.17(12) | 0.84(7) | SB2 | (10) |
| 26 Vul | 11.088 | 12.33(13) | 0.284(9) | 50.1(19) | 26492.61(5) | 0.205(6) | SB1 | (11) | |
| HD 203439 | 20.30 | 44.9(12) | 0.441(17) | 220(4) | 24363.56(11) | 1.87(12) | 1.08(7) | SB2 | (12) |
| 14 Peg | 5.30465(3) | 6.89(12) | 0.528(10) | 302.7(17) | 29117.474(13) | 0.0813(30) | 0.0746(29) | SB2 | (13) |
Notes.
Values of a sin i, M1sin3i, and M1sin3i for SB2 systems and a1 sin i and f(M) for SB1 systems were re-calculated using coefficients given by Torres et al. (2010). Therefore, they may slightly differ from those given in the cited papers.
Adopted from Maury (1922a).
References. References to orbital solutions: (1) Fekel et al. (2011), (2) Nordström et al. (1997), (3) Nariai (1970), (4) Evans (1969), (5) Hubrig et al. (2008), (6) Moore (1931b), (7) Popper (1943), (8) Kaufmann & Klippel (1973), (9) Norris (1949), (10) Harper (1928), (11) Shajn (1933), (12) Harper (1926), (13) Petrie (1940).
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