Pulsational instability of pre-main-sequence models from accreting protostars - II. Modelling echelle diagrams of δ Scuti stars without rotational splitting

Open Access

Table 3.

Percentage rate of extracted stellar parameters that agree with the model’s values within 1σ.

	χ²	χ²	χ²
		3σ	1σ	≤1	≤28.87
	(%)	(%)	(%)	(%)	(%)
Rayleigh limit corresponding to 27 day light curve
M_⋆	63	76	49	69	76
T_eff	73	83	37	16	64
log g	63	70	46	63	81
R	69	71	50	64	81
L	74	81	43	31	70
Age	71	77	57	61	84
Z	64	71	59	71	64

Total	68	75	49	54	74

Rayleigh limit corresponding to 108 day light curve
M_⋆ (M_⊙)	71	77	49	47	74
T_eff (K)	71	81	39	13	67
log g	69	67	43	46	79
R (R_⊙)	69	73	44	40	79
L (L_⊙)	74	81	43	16	67
Age (Myr)	74	79	46	40	71
Z	70	77	56	64	64

Total	71	76	48	38	72

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.