Table 1.

The parameters used in the current study for the late-type stars with different effective temperatures Teff, gravity log g, and the acoustic wave energy flux Fac computed for each star.

StarBVTefflog gFac
(mag)(K)(erg cm−2 s−1)
F8V0.4661604.3552.5E8
G0V0.5859434.3601.6E8
G2V0.6558114.3681.3E8
G5V0.6856574.4438.5E7
K2V0.8950554.5581.8E7
M0V1.4038504.7833.4E5
StarBVTefflog gFac
(mag)(K)(erg cm−2 s−1)
F8V0.4661604.3552.5E8
G0V0.5859434.3601.6E8
G2V0.6558114.3681.3E8
G5V0.6856574.4438.5E7
K2V0.8950554.5581.8E7
M0V1.4038504.7833.4E5
Table 1.

The parameters used in the current study for the late-type stars with different effective temperatures Teff, gravity log g, and the acoustic wave energy flux Fac computed for each star.

StarBVTefflog gFac
(mag)(K)(erg cm−2 s−1)
F8V0.4661604.3552.5E8
G0V0.5859434.3601.6E8
G2V0.6558114.3681.3E8
G5V0.6856574.4438.5E7
K2V0.8950554.5581.8E7
M0V1.4038504.7833.4E5
StarBVTefflog gFac
(mag)(K)(erg cm−2 s−1)
F8V0.4661604.3552.5E8
G0V0.5859434.3601.6E8
G2V0.6558114.3681.3E8
G5V0.6856574.4438.5E7
K2V0.8950554.5581.8E7
M0V1.4038504.7833.4E5
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