Table 2: The physical parameters of the two programme stars. The mass and radius are given in solar units; $v\sin~i$ and $v_{\rm crit}$ are given in km s^-1.
Star $\log~T_{\rm eff}$ $\log~g$ Mass Radius $\log(L/L_\odot)$ $M_{\rm bol}$ $v\sin~i$ $v_{\rm crit}$

HD 106419 $4.089\pm0.010$ $3.42\pm0.15$ $4.7\pm0.5$ $6.8\pm0.5$ $2.99\pm0.15$ $-2.71\pm0.15$ $78\pm4$ 297

HD 121190 $4.082\pm0.010$ $4.43\pm0.09$ $2.8\pm0.3$ $1.7\pm0.3$ $1.75\pm0.10$ $0.39\pm0.10$ $118\pm3$ 458

**Table 2:** The physical parameters of the two programme stars. The mass and radius are given in solar units; $v\sin~i$ and $v_{\rm crit}$ are given in km s^-1.
Star	$\log~T_{\rm eff}$	$\log~g$	Mass	Radius	$\log(L/L_\odot)$	$M_{\rm bol}$	$v\sin~i$	$v_{\rm crit}$
HD 106419	$4.089\pm0.010$	$3.42\pm0.15$	$4.7\pm0.5$	$6.8\pm0.5$	$2.99\pm0.15$	$-2.71\pm0.15$	$78\pm4$	297
HD 121190	$4.082\pm0.010$	$4.43\pm0.09$	$2.8\pm0.3$	$1.7\pm0.3$	$1.75\pm0.10$	$0.39\pm0.10$	$118\pm3$	458

Source LaTeX | All tables | In the text

	1 Introduction
	2 Data description
	3 Physical parameters
	4 Frequency analysis
	5 Discussion
	References