Table 10.
Adopted spectroscopic solutions of the SB1 systems in the MONOS sample.
| Name | SBS Classification |
Period | T0 | e | ω | K1 | γ1 | f(m) | v sin i | Ref | |
|---|---|---|---|---|---|---|---|---|---|---|---|
| MONOS I | MONOS II | d | JD−2 400 000 | degrees | km s−1 | km s−1 | M⊙ | km s−1 | |||
| HD 164 438 | SB1 | SB1 | 10.249 74(17) | 55 501.114(74) | 0.296(13) | 220.7(26) | 27.78(40) | -14.4(25) | 0.0198(9) | 55(3) | TP. HeI |
| V479 Sct | SB1 | SB1 | 3.906 09(12) | 55 017.468(240) | 0.272(107) | 263.5(270) | 19.73(243) | 26.52(185) | 0.002 77(105) | 157(8) | TP. OIII |
| Cyg X-1 | SB1 | SB1E | 5.599 74(f) | 56 792.37(11) | 0.0(f) | ... | 83.81(128) | 2.66(11) | 0.341 | 95(5) | TP. HeII |
| BD +36 4063 | SB1 | SB1E† | 4.812 17(3) | 58 381.04(2) | 0.01(1) | 22.0(83) | 160.0(3) | 0.5(18) | 2.06(10) | 96(5) | TP. comb. HeII |
| HDE 229 234 | SB1 | SB1E† | 3.510 395(12) | 56 527.114(13) | 0.04(1) | 56.0(20) | 49.9(6) | -29.6(5) | 0.0451(16) | 95(5) | TP. comb. HeI |
| ALS 15 133 | SB1 | SB1 unc. | 2 259.0(46) | 53 355.0(134) | 0.34(11) | 157.9(260) | 9.0(1) | -13.0(1) | 0.1419 * | ... | Ko12 |
| Cyg OB2-A11 | SB1 | SB1 | 15.442 8(25) | 55 761.47(99) | 0.136(59) | 47.0(24) | 23.4(14) | -18.58(99) | 0.0199(37) | 100(7) | TP. comb. HeI |
| Cyg OB2-22 B | SB1 | SB1 unc. | 38.0(2) | 56 719.9(16) | 0.21(20) | 244.0(31) | 9.5(17) | -20.4(12) | 0.0032 * | ... | Ko14 |
| Cyg OB2-41 | SB1 | SB1 | 29.370 3(49) | 56 542.66(91) | 0.21(5) | 255.0(12) | 41.8(15) | -2.4(12) | 0.208(29) | ... | TP. comb. HeI |
| ALS 15 148 | SB1 | SB1E† | 3.170 36(11) | 58 679.22(9) | 0.06(5) | 71.0(49) | 28.3(13) | -6.9(9) | 0.0074(11) | 177(9) | TP. comb. HeI |
| Cyg OB2-1 | SB1+Ca | SB1E+Ca | 4.852 24(21) | 56 338.35(29) | 0.17(7) | 238.0(200) | 69.9(45) | -27.5(32) | 0.164(33) | 203(10) | TP. comb. HeI |
| ALS 15 131 | SB1 | SB1 unc. | 4.625 2(12) | 55 971.8(67) | 0.15(15) | 240.0(52) | 5.4(9) | -17.4(6) | 0.0001 * | ... | Ko14 |
| Cyg OB2-20 | SB1 | SB1 | 25.125 2(11) | 53 922.81(22) | 0.375(22) | 124.0(41) | 43.0(12) | -11.13(81) | 0.164(14) | 14(1) | TP. comb. HeI |
| Cyg OB2-70 | SB1 | SB1 unc. | 245.1(3) | 56 549.1(84) | 0.51(17) | 242.0(16) | 14.5(29) | -17.8(14) | 0.049 * | ... | Ko14 |
| Cyg OB2-15 | SB1 | SB1 | 14.657 47(38) | 52 162.41(54) | 0.138(36) | 53.0(14) | 40.0(13) | -10.2(10) | 0.095(11) | 163(8) | TP. comb. HeI |
| ALS 15 115 | SB1 | SB1 unc. | 4066.0(45) | 52 229.0(29) | 0.75(f) | 352.0(9) | 15.0(23) | -12.1(11) | 0.412 * | ... | Ko14 |
| Cyg OB2-29 | SB1 | SB1 unc. | 151.2(8) | 56 543.7(38) | 0.60(20) | 15.0(10) | 17.5(23) | -10.7(8) | 0.043 * | ... | Ko14 |
| Cyg OB2-11 | SB1 | SB1 | 72.488(50) | 54 925.4(11) | 0.374(58) | 269.4(72) | 23.5(11) | -27.1(8) | 0.078(16) | 75(3) | TP. comb. HeI |
| V747 Cep | SB1E | SB1E | 5.332 37(15) | 54 401.172 3(1367) | 0.37(3) | 180.2(65) | 99.6(36) | -10.7(25) | 0.436(49) | 220(11) | TP. HeII |
| HD 12 323 | SB1 | SB1E† | 1.925 14(6) | 56 229.34(2) | 0.0(f) | ... | 29.82(221) | -46.1(12) | 0.0053(12) | 121(6) | TP. comb. CC |
| HD 16 429 Aa | SB1+Ca | SB1E+Cas | 3.054 42(f) | 51 893.22(10) | 0.17(4) | 169.0(12) | 136.0(6) | -50.0(3) | 0.76(1) | ... | Mc03 |
| HD 15 137 | SB1 | SB1 | 55.399 4(30) | 40 017.483(819) | 0.585 2(267) | 153.18(351) | 13.92(57) | -41.67(32) | 0.0082(16) | 270(14) | TP. HeI+HeII |
| HD 14 633 AaAb | SB1+Ca? | SB1+Ca | 15.409 24(8) | 51 792.635(32) | 0.695(13) | 139.6(14) | 19.1(3) | -41.55(16) | 0.0041(3) | 121(6) | TP. comb. HeI |
| HD 37 737 | SB1 | SB1E | 7.847 031(32) | 56 342.54(63) | 0.407(21) | 161.0(32) | 70.8(22) | -9.4(10) | 0.220(21) | 201(11) | TP. comb. CC |
| 15 Mon Aa | SB1a | SB2a | 27 112.2(14819) | 50 105.48(151 941) | 0.716(98) | 69.2(111) | 13.0(1) | 33.6(10) | 2.12 | ... | Cv10 |
| HD 46 573 | SB1 | SB1 | 10.653 9(f) | 53 732.53(14) | 0.63(3) | 265.04(720) | 11.2(5) | 50.1(4) | 0.000 7(1) | 77(3) | TP. comb. HeI |
| θ1 Ori CaCb | SB1?+Sa | SB1+Sa | 4201.0(200) | 56 546.0(107) | 0.546(90) | 85.9(146) | 15.2(19) | 29.3(9) | 0.9(4) | 23(2) | TP. OIII |
| HD 52 533 A | SB1 | SB1E | 21.965 2(14) | 44 615.34(76) | 0.364(55) | 337.8(82) | 82.2(44) | 39.25(324) | 1.02(17) | 299(15) | TP. comb. CC |
Notes. The T0 values correspond to the periastron passage for the eccentric orbits. Errors are in parentheses, corresponding to the last digits. An “f” means that the parameter was fixed for that solution. An asterisk after the mass function indicates that the value was calculated by us with the parameters of the orbital solution. We denote ellipsoidal systems with an “†” after the SBS classification.
References. (Ko12) Kobulnicky et al. (2012) ; (Ko14) Kobulnicky et al. (2014) ; (Mc03) McSwain (2003) ; (Cv10) Cvetković et al. (2010); (TP) This work.
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