Table 3
Parameters of individual subluminous stars in binaries.
| Star | Teff | M | R∗ | a | Obs. Ṁ | Pred. Ṁ | L X | Comp.a | Source | |||||||
| [K] | [M⊙] | [R⊙] | [R⊙] | [M⊙ yr-1] | [M⊙ yr-1] | [erg s-1] | ||||||||||
|
|
||||||||||||||||
| PG0101+039 (Feige 11) | 27 300 | 0.47 | 0.19 | 3.1 | no wind | WD | 1, 2 | |||||||||
| GD 687 | 24 400 | 0.47 | 0.25 | 2.3 | no wind | WD | 3 | |||||||||
| ϕ Per (HD 10516, HR 496) | 53 000 | 1.14 | 1.3 | 232 | 2.7 × 10-9 | B1.5Ve | 4 | |||||||||
| BD+37°442 | 48 000 | 0.9 | 1.6 | 3 × 10-9 | 2.4 × 10-9 | 2.3 × 1031 | WD | 5, 6 | ||||||||
| CPD −71°172 | 55 000 | 0.5 | 0.24 | 1.8 × 10-10 | F3-F4IV | 7 | ||||||||||
| HFG 1 (V664 Cas) | 83 000 | 0.57 | 0.19 | 3.5 | 2.4 × 10-9 | 3.2 × 1030 | F-K | 8, 9 | ||||||||
| KPD 0422+5421 (IQ Cam) | 25 000 | 0.36 | 0.17 | 0.93 | no wind | WD | 10, 11 | |||||||||
| V1405 Ori | 35 100 | 0.47 | 0.17 | >2.1 | 1.9 × 10-14 | F-G | 12 | |||||||||
| LB 3459 (AA Dor) | 42 000 | 0.33 | 0.181 | 1.2153 | 8.3 × 10-13 | K | 13, 14 | |||||||||
| Albus 1 (CPD -20°1123) | 19 800 | 0.49 | 0.62 | >6.5 | 3.9 × 10-14 | 15 | ||||||||||
| HD 49798 | 47 500 | 1.5 | 1.45 | 7 | 3 × 10-9 | 2.7 × 10-9 | 3 × 1030 b | NS | 16, 17, 18, 69, 72 | |||||||
| BD+34°1543 | 36 700 | 0.47 | 0.14 | 447 | no wind | F | 19 | |||||||||
| HS 0705+6700 (V470 Cam) | 28 800 | 0.483 | 0.230 | 0.81 | no wind | M | 20 | |||||||||
| FY CMa (HD 58978) | 45 000 | 1.3 | 0.6 | 112 | 1.0 × 10-9 | B0.5IVe | 21 | |||||||||
| SDSS J08205+0008 | 26 100 | 0.251 | 0.15 | 0.588 | no wind | BD | 22 | |||||||||
| US 708 | 47 200 | 0.3 | 0.13 | 1 | 4.4 × 10-13 | WD | 23 | |||||||||
| TYC 7709-376-1 | 28 400 | 0.461 | 0.179 | 0.963 | no wind | dM | 24 | |||||||||
| EC 10246-2707 | 28 900 | 0.45 | 0.17 | 0.84 | no wind | dM | 25 | |||||||||
| Feige 34 (GJ 398.2) | 70 000 | 0.55 | 0.14 | 1.8 × 10-10 | 1.7 × 1030 | M | 26, 27 | |||||||||
| LSS 2018 (KV Vel) | 77 000 | 0.63 | 0.157 | 2.1 | 7.5 × 10-10 | M | 28, 29, 30 | |||||||||
| Feige 36 (WD 1101+249) | 29 700 | 0.45 | 0.12 | 2.4 | no wind | < 1.7 × 1030 | WD | 65, 66 | ||||||||
| PG1104+243 | 33 500 | 0.47 | 0.13 | 322 | no wind | G0 | 31 | |||||||||
| Feige 48 (KL UMa) | 29 900 | 0.46 | 0.215 | 2.1 | no wind | K | 10, 32, 33, 71 | |||||||||
| PG1232-136 | 26 900 | 0.45 | 0.16 | >4 | < 1 × 10-13 | no wind | < 5 × 1029 | BH | 42, 65 | |||||||
| BD+18°2647 (Feige 67) | 60 000 | 0.47c | 0.36 | 1.6 × 10-9 | < 3.2 × 1029 | 27, 34 | ||||||||||
| HW Vir (BD-07°3477) | 28 500 | 0.48 | 0.197 | 0.853 | no wind | dM | 35 | |||||||||
| CS 1246 | 28 450 | 0.39 | 0.19 | 19.6 | no wind | 37, 38 | ||||||||||
| Feige 80 | 37 500 | 0.43 | 0.14 | 530 | 1.1 × 10-14 | G1V | 26, 39 | |||||||||
| PG1336-018 (NY Vir) | 32 800 | 0.471 | 0.147 | 0.723 | no wind | dM | 40, 41 | |||||||||
| Feige 87 | 27 400 | 0.47 | 0.19 | 442 | no wind | G4V | 19 | |||||||||
| CD-30 11 223 | 29 200 | 0.47 | 0.169 | 0.599 | < 3 × 10-13 | no wind | < 1.5 × 1029 | WD | 42 | |||||||
| HD 128220 | 40 600 | 0.54 | 0.78 | 520 | 2 × 10-10 | 1.0 × 10-9 | G0III | 43, 44, 45, 70 | ||||||||
| PG1432+159 | 26 900 | 0.5 | 0.16 | no wind | < 9.8 × 1030 | NS | 66, 67, 68 | |||||||||
| 2M 1533+3759 | 29 200 | 0.376 | 0.166 | 0.98 | no wind | M5V | 46 | |||||||||
| PG1605+072 (V338 Ser) | 32 300 | 0.5 | 0.28 | 3.1 × 10-13 | 47 | |||||||||||
| SDSS J162256.66+473051.1 | 29 000 | 0.48 | 0.168 | 0.58 | no wind | BD | 48, 49 | |||||||||
| PG1718+519 | 29 000 | 0.5 | 0.12 | no wind | G4V | 50, 51 | ||||||||||
| MT Ser | 50 000 | 0.6 | 0.13 | 0.9 | 1.2 × 10-12 | dM | 64 | |||||||||
| BD+29°3070 | 28 500 | 0.47 | 0.19 | 586 | no wind | F5V | 19 | |||||||||
| V477 Lyr | 49 500 | 0.508 | 0.172 | 2.21 | 7.4 × 10-12 | M | 52 | |||||||||
| KIC 11558725 | 27 900 | 0.48 | 0.2 | 20.3 | no wind | WD | 53 | |||||||||
| KPD 1930+2752d | 35 200 | 0.47 | 0.18 | 0.98 | 3.4 × 10-14 | WD | 54, 55 | |||||||||
| 2M 1938+4603 | 29 600 | 0.372 | 0.196 | 0.823 | no wind | dM | 56, 57 | |||||||||
Notes.
Either a spectral type or WD for white dwarf, BD for brown dwarf, NS for neutron star, and BH for a black hole.
Reference. (1) Geier et al. (2008); (2) Napiwotzki (1999); (3) Geier et al. (2010a); (4) Gies et al. (1998); (5) La Palombara et al. (2012); (6) Jeffery & Hamann (2010); (7) Viton et al. (1988); (8) Shimanskii et al. (2004); (9) Montez et al. (2010); (10) Koen et al. (1998); (11) Orosz & Wade (1999); (12) Geier et al. (2014); (13) Rauch (2000); (14) Rauch & Werner (2003); (15) Vennes et al. (2007); (16) Kudritzki & Simon (1978); (17) Bisscheroux et al. (1997); (18) Mereghetti et al. (2013); (19) Vos et al. (2013); (20) Drechsel et al. (2001); (21) Peters et al. (2008); (22) Schaffenroth et al. (2011); (23) Geier et al. (2015); (24) Schaffenroth et al. (2013); (25) Barlow et al. (2013); (26) Thejll et al. (1995); (27) La Palombara et al. (2014); (28) Hilditch et al. (1996); (29) Aungwerojwit et al. (2007); (30) Ribeiro & Baptista (2011); (31) Vos et al. (2012); (32) Charpinet et al. (2005b); (33) Latour et al. (2014); (34) Deetjen (2000); (35) İbanoǧlu et al. (2004); (37) Barlow et al. (2010); (38) Barlow et al. (2011); (39) Barlow et al. (2012b); (40) Vučković et al. (2007); (41) Van Grootel et al. (2013); (42) Mereghetti et al. (2014); (43) Gruschinske et al. (1983); (44) Howarth & Heber (1990); (45) Rauch (1993); (46) For et al. (2010); (47) Heber et al. (1999); (48) Schaffenroth et al. (2014); (49) Kupfer et al. (2015); (50) Theissen et al. (1995); (51) Aznar Cuadrado & Jeffery (2002); (52) Afşar & Ibanoǧlu (2008); (53) Telting et al. (2012); (54) Maxted et al. (2000); (55) Geier et al. (2007); (56) Østensen et al. (2010); (57) Barlow et al. (2012a); (64) Green et al. (1984); (65) Geier et al. (2010b); (66) Mereghetti et al. (2011); (67) Saffer et al. (1994); (68) Maxtedet al. (2002); (69) Hamann (2010); (70) Hamann et al. (1981); (71) Fontaine et al. (2014); (72) Mereghetti et al. (2016).
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