|${\cal M}_{\rm a}d^{-2}$|, distance d of the observed stars, the averaged residual acceleration of the atmosphere in the epochs when the dynamical condition C(II) (Paper I) of QSAA is satisfied, mass, equilibrium luminosity and effective temperature, minimal and maximal radius, magnitude averaged absolute visual magnitude and averaged ‘static’ surface gravity.
. | |${\cal M}_{\rm a}d^{-2}\times 10^7$| . | d . | |$\overline{a^{\rm (dyn)}}$| . | |${\cal M}_{\rm a}$| . | Leq . | Teq . | Rmin, Rmax . | 〈MV〉 . | gs . |
---|---|---|---|---|---|---|---|---|---|
. | (M⊙ pc−2) . | (pc) . | (m s−2) . | (M⊙) . | (L⊙) . | (K) . | (R⊙) . | (mag) . | (m s−2) . |
SWAnda | 7.00 ± 0.76 | 626 ± 31 | 0.27 | 0.26 ± 0.04 | 39.8 ± 4 | 6644 | 4.51, 5.05 | 0.710 | 3.09 |
SWAndb | 1.685 | 41.5 ± 4 | 6672 | 4.53, 5.06 | 0.68 | 3.02 | |||
SWAndc | 41.8 ± 4 | 6690 | 4.44, 5.05 | 0.655 | |||||
SU Drad | 663 ± 67 | 0.68 ± 0.03 | 45.9 ± 9.3 | 6813 | 4.46, 5.29 | 0.68 | 8.3 | ||
DH Pege | 9.20 ± 0.32 | 893 ± 104 | −0.03 | 0.73 ± 0.09 | 123 ± 27 | 7464 | 6.40, 7.06 | 0.02 | 4.50 |
DY Peg | 2.42 ± 0.27 | 817 ± 24 | 1.40 | 1.40 ± 0.24 | 34.6 ± 2.1 | 7177 | 3.74, 3.95 | 0.84 | 30.2 |
CU Com | 1.28 ± 0.21 | 3059 ± 181 | 0.02 | 0.55 ± 0.03 | 39.0 ± 4.7 | 6942 | 3.95, 4.70 | 0.82 | 8.00 |
V372 Ser f | 6.12 ± 0.31 | 964 ± 81 | 0.41 | 0.57 ± 0.10 | 21.9 ± 5.2 | 6722 | 4.07, 4.40 | 1.58 | 12.9 |
V500 Hya f | 40.3 ± 6.7 | 467 ± 16 | 2.40 | 0.88 ± 0.06 | 8.97 ± 1.23 | 6924 | 1.97, 2.05 | 2.40 | 54.8 |
. | |${\cal M}_{\rm a}d^{-2}\times 10^7$| . | d . | |$\overline{a^{\rm (dyn)}}$| . | |${\cal M}_{\rm a}$| . | Leq . | Teq . | Rmin, Rmax . | 〈MV〉 . | gs . |
---|---|---|---|---|---|---|---|---|---|
. | (M⊙ pc−2) . | (pc) . | (m s−2) . | (M⊙) . | (L⊙) . | (K) . | (R⊙) . | (mag) . | (m s−2) . |
SWAnda | 7.00 ± 0.76 | 626 ± 31 | 0.27 | 0.26 ± 0.04 | 39.8 ± 4 | 6644 | 4.51, 5.05 | 0.710 | 3.09 |
SWAndb | 1.685 | 41.5 ± 4 | 6672 | 4.53, 5.06 | 0.68 | 3.02 | |||
SWAndc | 41.8 ± 4 | 6690 | 4.44, 5.05 | 0.655 | |||||
SU Drad | 663 ± 67 | 0.68 ± 0.03 | 45.9 ± 9.3 | 6813 | 4.46, 5.29 | 0.68 | 8.3 | ||
DH Pege | 9.20 ± 0.32 | 893 ± 104 | −0.03 | 0.73 ± 0.09 | 123 ± 27 | 7464 | 6.40, 7.06 | 0.02 | 4.50 |
DY Peg | 2.42 ± 0.27 | 817 ± 24 | 1.40 | 1.40 ± 0.24 | 34.6 ± 2.1 | 7177 | 3.74, 3.95 | 0.84 | 30.2 |
CU Com | 1.28 ± 0.21 | 3059 ± 181 | 0.02 | 0.55 ± 0.03 | 39.0 ± 4.7 | 6942 | 3.95, 4.70 | 0.82 | 8.00 |
V372 Ser f | 6.12 ± 0.31 | 964 ± 81 | 0.41 | 0.57 ± 0.10 | 21.9 ± 5.2 | 6722 | 4.07, 4.40 | 1.58 | 12.9 |
V500 Hya f | 40.3 ± 6.7 | 467 ± 16 | 2.40 | 0.88 ± 0.06 | 8.97 ± 1.23 | 6924 | 1.97, 2.05 | 2.40 | 54.8 |
The estimated errors of |$[M/\text{H}]$|, Teq and 〈MV〉 are |$\pm 0.1\,\mbox{dex}, 25\mbox{ K}\text{ and } 0.25\mbox{ mag}$|, respectively; |$g_{\rm s}=G{\cal M}\overline{R}^{-2}$|.
aHJD−2454350 = 0, 1, 3.
bHJD−2454830 = −8, −1, 0, 1, 2, |${\cal M}_{\rm a}$|, d of a were used.
cHJD−2444720 = 0, 1, 3, 4, |${\cal M}_{\rm a}$|, d of a were used.
dPaper I.
eThe data were determined from the photometry on HJD = 2454349, see the text.
fPaper II.
|${\cal M}_{\rm a}d^{-2}$|, distance d of the observed stars, the averaged residual acceleration of the atmosphere in the epochs when the dynamical condition C(II) (Paper I) of QSAA is satisfied, mass, equilibrium luminosity and effective temperature, minimal and maximal radius, magnitude averaged absolute visual magnitude and averaged ‘static’ surface gravity.
. | |${\cal M}_{\rm a}d^{-2}\times 10^7$| . | d . | |$\overline{a^{\rm (dyn)}}$| . | |${\cal M}_{\rm a}$| . | Leq . | Teq . | Rmin, Rmax . | 〈MV〉 . | gs . |
---|---|---|---|---|---|---|---|---|---|
. | (M⊙ pc−2) . | (pc) . | (m s−2) . | (M⊙) . | (L⊙) . | (K) . | (R⊙) . | (mag) . | (m s−2) . |
SWAnda | 7.00 ± 0.76 | 626 ± 31 | 0.27 | 0.26 ± 0.04 | 39.8 ± 4 | 6644 | 4.51, 5.05 | 0.710 | 3.09 |
SWAndb | 1.685 | 41.5 ± 4 | 6672 | 4.53, 5.06 | 0.68 | 3.02 | |||
SWAndc | 41.8 ± 4 | 6690 | 4.44, 5.05 | 0.655 | |||||
SU Drad | 663 ± 67 | 0.68 ± 0.03 | 45.9 ± 9.3 | 6813 | 4.46, 5.29 | 0.68 | 8.3 | ||
DH Pege | 9.20 ± 0.32 | 893 ± 104 | −0.03 | 0.73 ± 0.09 | 123 ± 27 | 7464 | 6.40, 7.06 | 0.02 | 4.50 |
DY Peg | 2.42 ± 0.27 | 817 ± 24 | 1.40 | 1.40 ± 0.24 | 34.6 ± 2.1 | 7177 | 3.74, 3.95 | 0.84 | 30.2 |
CU Com | 1.28 ± 0.21 | 3059 ± 181 | 0.02 | 0.55 ± 0.03 | 39.0 ± 4.7 | 6942 | 3.95, 4.70 | 0.82 | 8.00 |
V372 Ser f | 6.12 ± 0.31 | 964 ± 81 | 0.41 | 0.57 ± 0.10 | 21.9 ± 5.2 | 6722 | 4.07, 4.40 | 1.58 | 12.9 |
V500 Hya f | 40.3 ± 6.7 | 467 ± 16 | 2.40 | 0.88 ± 0.06 | 8.97 ± 1.23 | 6924 | 1.97, 2.05 | 2.40 | 54.8 |
. | |${\cal M}_{\rm a}d^{-2}\times 10^7$| . | d . | |$\overline{a^{\rm (dyn)}}$| . | |${\cal M}_{\rm a}$| . | Leq . | Teq . | Rmin, Rmax . | 〈MV〉 . | gs . |
---|---|---|---|---|---|---|---|---|---|
. | (M⊙ pc−2) . | (pc) . | (m s−2) . | (M⊙) . | (L⊙) . | (K) . | (R⊙) . | (mag) . | (m s−2) . |
SWAnda | 7.00 ± 0.76 | 626 ± 31 | 0.27 | 0.26 ± 0.04 | 39.8 ± 4 | 6644 | 4.51, 5.05 | 0.710 | 3.09 |
SWAndb | 1.685 | 41.5 ± 4 | 6672 | 4.53, 5.06 | 0.68 | 3.02 | |||
SWAndc | 41.8 ± 4 | 6690 | 4.44, 5.05 | 0.655 | |||||
SU Drad | 663 ± 67 | 0.68 ± 0.03 | 45.9 ± 9.3 | 6813 | 4.46, 5.29 | 0.68 | 8.3 | ||
DH Pege | 9.20 ± 0.32 | 893 ± 104 | −0.03 | 0.73 ± 0.09 | 123 ± 27 | 7464 | 6.40, 7.06 | 0.02 | 4.50 |
DY Peg | 2.42 ± 0.27 | 817 ± 24 | 1.40 | 1.40 ± 0.24 | 34.6 ± 2.1 | 7177 | 3.74, 3.95 | 0.84 | 30.2 |
CU Com | 1.28 ± 0.21 | 3059 ± 181 | 0.02 | 0.55 ± 0.03 | 39.0 ± 4.7 | 6942 | 3.95, 4.70 | 0.82 | 8.00 |
V372 Ser f | 6.12 ± 0.31 | 964 ± 81 | 0.41 | 0.57 ± 0.10 | 21.9 ± 5.2 | 6722 | 4.07, 4.40 | 1.58 | 12.9 |
V500 Hya f | 40.3 ± 6.7 | 467 ± 16 | 2.40 | 0.88 ± 0.06 | 8.97 ± 1.23 | 6924 | 1.97, 2.05 | 2.40 | 54.8 |
The estimated errors of |$[M/\text{H}]$|, Teq and 〈MV〉 are |$\pm 0.1\,\mbox{dex}, 25\mbox{ K}\text{ and } 0.25\mbox{ mag}$|, respectively; |$g_{\rm s}=G{\cal M}\overline{R}^{-2}$|.
aHJD−2454350 = 0, 1, 3.
bHJD−2454830 = −8, −1, 0, 1, 2, |${\cal M}_{\rm a}$|, d of a were used.
cHJD−2444720 = 0, 1, 3, 4, |${\cal M}_{\rm a}$|, d of a were used.
dPaper I.
eThe data were determined from the photometry on HJD = 2454349, see the text.
fPaper II.
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