Table 6
Linear rates of period change, measured by RV template fitting (extract).
Star | ![]() |
![]() |
Notes |
---|---|---|---|
AA Gem | −1.721 | 0.102 | |
AC Mon | −0.453 | 0.294 | Nlit = 1 |
AH Vel | 0.238 | 0.091 | non-linear |
AK Cep | −0.234 | 0.759 | |
AN Aur | 2.978 | 0.548 | non-lin? |
AO CMa | 0.185 | 0.014 | Nlit = 1, 3 points |
AQ Car | −0.669 | 0.031 | non-linear |
AQ Pup | 26.128 | 5.126 | non-linear |
AV Cir | 0.228 | 0.033 | |
AV Sgr | 36.292 | 46.894 | noisy |
... |
Notes. The full table listing all 146 Cepheids is available via the CDS. is measured at a significance exceeding 3σ for 80 (shown in Fig. 27. Nlit = 1 indicates that only one older literature epoch was available. ‘non-lin?’ indicates possible signs for non-linear period changes, ‘nonlinear’ indicates clear evidence for this. ‘noisy’ marks Δϕ sequences exhibiting high scatter. ‘3 points’ highlight stars with only few (3) epochs for determining
. ‘biased’ indicates results where the fit result may be affected by non-linear trends or uneven weights; ‘biased?’ indicates results where this is less clearly the case.
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