Similar additional frequency patterns on fundamental- and overtone-mode RR Lyrae stars showing f68 frequencies

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Table 2.

Modelling input parameters of the studied stars.

Star	M ^(a)	T_eff	L_bol	Z ^(b)
	(M_⊙)	(K)	(L_⊙)
KIC 9658012	0.5281	6464 ± 100 ^(*)	36 ± 5	0.0011
V894 Cyg	0.63089	6330 ± 100 ^(*)	42 ± 2	0.0004
V346 Lyr	0.72084	6205 ± 100 ^(*)	43 ± 7	0.0003
V1510 Cyg	0.66043	6393 ± 200 ^(* *)	46 ± 4	0.0003
EPIC 60018644	0.72600	6333 ± 200 ^(* *)	54 ± 8	0.0003

Notes.

^(a)

Interpolated on linear non-adiabatic period–mass grids.

^(b)

Hydrogen content is assumed to be X = 0.754.

^(*)Temperature calculations are based on Gaia mean colours, [Fe/H], and spectroscopy.

^(* *)Temperature calculation is only based on Gaia mean colours and [Fe/H].

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