Table 1: Calculated models of NRP for the test star pulsating with the frequency 15 cycle/day.
Set $\ell$ |m| i Fluctuation
$P_{\rm r} = 6.4$ h
1 4 4 60$^\circ $ $\Delta~T/T=10$%
$P_{\rm r} = 14.4$ h
2 9 9 60$^\circ $ $\Delta~T/T=10$%
3 9 9 60$^\circ $ $\Delta~v=3$ km s-1
4 9 9 60$^\circ $ $\Delta~v=10$ km s-1
$P_{\rm r} = 4.8$ h
5 5 3 55$^\circ $ $\Delta~T/T=10$%
6 5 3 70$^\circ $ $\Delta~T/T=10$%
7 5 3 85$^\circ $ $\Delta~T/T=10$%
8 5 3 55$^\circ $ $\Delta~v=10$ km s-1
9 5 3 70$^\circ $ $\Delta~v=10$ km s-1
10 5 3 85$^\circ $ $\Delta~v=10$ km s-1
$P_{\rm r} = 6.4$ h
11 5 4 55$^\circ $ $\Delta~T/T=10$%
12 5 4 85$^\circ $ $\Delta~T/T=10$%
13 5 4 55$^\circ $ $\Delta~v=10$ km s-1
14 5 4 85$^\circ $ $\Delta~v=10$ km s-1


Source LaTeX | All tables | In the text