The nature of the line profile variability in the spectrum of the massive binary HD 152219

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Table 4:

Physical parameters of the known and suspected non-radial pulsators.
Object	Sp.Type	$\log\frac{L}{L_\odot}$	$\log T_{\rm eff}$	$\log g$	Status^a
			(K)	(cm s^-2)
HD 93521	O9.5V	4.62	4.48	3.92	C
$\zeta$ Oph	O9V	4.72	4.50	3.92	C
HD 152219^b	O9.5III	5.21	4.50	3.51	N
$\xi$ Per	O7.5III	5.36	4.52	3.59	C
HD 152249	O9I	5.54	4.47	3.23	S
$\lambda$ Cep	O6I	5.78	4.55	3.48	C
$\zeta$ Pup	O5I	5.87	4.59	3.57	S

^a C: confirmed NRPs, S: suspected NRPs, N: no NRP;
^b only the primary component is considered here.

Source LaTeX | All tables | In the text

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