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Table 6.

Properties of oscillating stars.

Source Mass ( * ) Mass L Teff cLT Δν
(M) (M) (L) (K) (μHz)
N77-135 2.003 1.99 ± 0.01 33.58 ± 1.10 6657 ± 288 0.10
N77-148 1.993 2.02 ± 0.01 40.24 ± 1.48 7284 ± 331 0.38
N77-151 1.991 1.99 ± 0.01 31.00 ± 1.07 7244 ± 324 0.33
N77-177 1.991 2.02 ± 0.01 38.99 ± 1.30 6945 ± 318 0.16
N77-186 1.984 1.99 ± 0.01 32.69 ± 1.18 7419 ± 319 0.43
N77-199 1.961 1.97 ± 0.02 26.74 ± 1.12 7662 ± 340 0.58
N77-202 1.988 1.99 ± 0.01 31.50 ± 1.35 7695 ± 338 0.65
N77-210 1.991 1.98 ± 0.02 27.87 ± 1.18 7803 ± 321 0.62 23
N77-240 1.960 1.95 ± 0.01 21.11 ± 0.73 7299 ± 318 0.38
N77-250 1.991 1.98 ± 0.02 28.18 ± 1.06 7471 ± 328 0.48
N77-255 2.001 1.97 ± 0.03 20.86 ± 0.66 6588 ± 271 −0.03 26
N77-319 1.851 1.88 ± 0.04 15.54 ± 0.52 6964 ± 305 0.19
N77-320 1.961 1.96 ± 0.01 22.54 ± 0.80 7422 ± 306 0.42
N77-325 1.860 1.85 ± 0.04 15.33 ± 0.62 7624 ± 323 0.58 32
N77-342 1.915 1.87 ± 0.04 15.83 ± 0.58 7531 ± 314 0.51 30
N77-438 1.79 1.82 ± 0.05 13.44 ± 0.45 6924 ± 300 0.14

Notes. The error in L and Teff is the square root of diagonal elements of covariance matrix and the cLT represent the correlation coefficient between L and Teff. Δν is the derived mean frequency separation and we adopt an error of 2 μHz on these values (Sect. 7.4.1). ( * )Mass determined using asteroseismic modelling.

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