Discovery of non-radial pulsations in the spectroscopic binary Herbig Ae star RS Chamaeleontis

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Table 11:

Frequency search and mode identification. Summary of the main results for the dominant frequencies of each component.
Primary component
	d^-1	Identification FPF	Identification^b F2D
		best^a ( $\ell$ , m)
f₁	21.11	(11, 11), (11, 9), (10, 6)	$\ell$ = 8-10
f₂	30.38	(10, 6), (9, 5), (11, 7)
Secondary component
	d^-1	Identification FPF	Identification^b F2D
		best^a ( $\ell$ , m)
f₁	12.81	(2, 1), (2, 2)	$\ell$ = 2 or 3
f_2b	19.11	(13, 5), (10, 5)	$\ell$ = 0
f₃	24.56	(6, 3), (6, 5)

^a The ( $\ell$ , m) couples indicated for the FPF method correspond to the best identification, in decreasing order.
^b For each of the frequencies detected by the FPF method, we identified an $\ell$ value as detected by the F2D method.

Source LaTeX | All tables | In the text

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