Table 3
Parameters determined previously (left) and our results (right) for the system TU UMa.
Study | Saha & White (1990a) | Kiss et al. (1995) | Wade et al. (1999) C | Model 1 | Model 2 |
|
|||||
Ppuls(M0) [d] | 0.5576581097 | 0.5576581097 | 0.55765817(29)D | 0.557657598![]() |
0.557657477![]() |
M0 [HJD] | 2 425 760.4364 | 2 425 760.4364 | 2 425 760.464(5)D | 2 442 831.4869![]() |
2 442 831.4864![]() |
Ṗ puls | × | −31.48∗ | −10.4(7)∗ |
![]() |
![]() |
10-11[d d-1] | |||||
a3 = 1/2 PpulsṖpuls | × | −8.78∗ | −2.9(2) |
![]() |
![]() |
10-11[d cycle-1] | |||||
β = Ṗpuls [ms yr-1] | × | −9.934∗ | −3.3(2)∗ |
![]() |
![]() |
β = Ṗpuls [d Myr-1] | × | −0.11498∗ | −0.038(3)∗ |
![]() |
![]() |
Porbit [yr] | 20.19∗ | 24.1(3)∗ | 23.27(24)∗ | 23.30![]() |
23.27![]() |
T0 [HJD] | 2 425 000∗ | 2 447 200(50) | 2 421 585(207) | 2 447 092![]() |
2 447 124![]() |
e | 0.970 | 0.90(5) | 0.74(10) | 0.663![]() |
0.686![]() |
ω [°] | 196.1∗ | 178(3) | 183(5)∗ | 181.3![]() |
184.1![]() |
A [light day] | 0.056 | 0.023(5)∗ | 0.0203(35)∗ | 0.0168![]() |
0.0172![]() |
a1sini [au] | 10 | 4.0(7)∗ | 3.52(61) | 2.91![]() |
2.99![]() |
f(M) [M⊙] | − | 0.11(1) | 0.080 | 0.046![]() |
0.049![]() |
M2,min ∗ [M⊙] | − | 0.17 | − | 0.327![]() |
0.339![]() |
K1 [km s-1] | 60.7∗ | 11.4(5) | 6.6 | 4.97![]() |
5.25![]() |
![]() |
− | − | − | 1.05(9) | 1.03(10) |
N max | ~ 43 | ~ 42 | 67 | 253 | 220 |
Notes. The mass limit of the second body was estimated from the mass function f(M), the orbit inclination (i = 90°), and the mass of the RR Lyrae star M1 = 0.55 M⊙ adopted from Fernley (1993) and Skarka (2014). Our parameters (right part of the table) were calculated from all maxima timings for model 1 and only from photoelectric, CCD, and DSLR measurements for model 2.
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