Table 1: Altair observed frequencies (from Paper I). From left to right, columns provide frequencies in cd^-1, in $\mu\mbox{Hz}$ , amplitudes in ppm, and finally, f₁/f_j=2,...,7 frequency ratios.
(c/d) ( $\mu\mbox{Hz}$ ) A (ppm) $f_1/f_{j\neq1}$

f₁ 15.768 182.50 413

f₂ 20.785 240.56 373 0.759

f₃ 25.952 300.37 244 0.607

f₄ 15.990 185.07 225 0.986

f₅ 16.182 187.29 139 0.974

f₆ 23.279 269.43 111 0.677

f₇ 28.408 328.80 132 0.555

**Table 1:** Altair observed frequencies (from Paper I). From left to right, columns provide frequencies in cd^-1, in $\mu\mbox{Hz}$ , amplitudes in ppm, and finally, f₁/f_j=2,...,7 frequency ratios.
	(c/d)	( $\mu\mbox{Hz}$ )	A (ppm)	$f_1/f_{j\neq1}$
f₁	15.768	182.50	413
f₂	20.785	240.56	373	0.759
f₃	25.952	300.37	244	0.607
f₄	15.990	185.07	225	0.986
f₅	16.182	187.29	139	0.974
f₆	23.279	269.43	111	0.677
f₇	28.408	328.80	132	0.555

Source LaTeX | All tables | In the text

	1 Introduction
	2 Fundamental parameters
	3 Modelling the star
	4 Comparison between theory and observations
	5 Conclusions
	References