Table 12: Astrophysical data for HD 92024. $M_{\rm bol,\odot } =4.75$ is assumed, and $M_{\odot } = 1.989\times 10^{30}$ kg and $G= 6.67259\times 10^{-11}$ m³ kg^-1 s^-2 are from Seidelmann (1992). Bolometric corrections are from Flower (1996).
Star A Star B

$M/{M}_{\odot}$ 15.0^+3.0_-4.0 3.0 $\pm$ 0.5

$R/{R}_{\odot}$ 8.37 $\pm$ 0.8 2.10 $\pm$ 0.4

$\log g$ (cgs) 3.77 $\pm$ 0.08 4.27 $\pm$ 0.18

$V_{\rm sync}\sin i$ (km s^-1) 51 $\pm$ 5 13 $\pm$ 3

Measured rotation (km s^-1) 75 $\pm$ 20

$\log T_{\rm eff}$ $4.407\pm0.009$ $4.097\pm0.035$

$\log~L/{L}_{\odot}$ 4.41 $\pm$ 0.09 1.96 $\pm$ 0.22

$M_{\rm bol}$ -6.28 $\pm$ 0.22 -0.14 $\pm$ 0.55

B.C. -2.45 -0.79

M_V -3.83 $\pm$ 0.25 0.65 $\pm$ 0.52

(m-M) 12.23 $\pm$ 0.22

Distance (pc) 2800 $\pm$ 300

**Table 12:** Astrophysical data for HD 92024. $M_{\rm bol,\odot } =4.75$ is assumed, and $M_{\odot } = 1.989\times 10^{30}$ kg and $G= 6.67259\times 10^{-11}$ m³ kg^-1 s^-2 are from Seidelmann (1992). Bolometric corrections are from Flower (1996).
	Star A	Star B
$M/{M}_{\odot}$	15.0^+3.0_-4.0	3.0 $\pm$ 0.5
$R/{R}_{\odot}$	8.37 $\pm$ 0.8	2.10 $\pm$ 0.4
$\log g$ (cgs)	3.77 $\pm$ 0.08	4.27 $\pm$ 0.18
$V_{\rm sync}\sin i$ (km s^-1)	51 $\pm$ 5	13 $\pm$ 3
Measured rotation (km s^-1)	75 $\pm$ 20
$\log T_{\rm eff}$	$4.407\pm0.009$	$4.097\pm0.035$
$\log~L/{L}_{\odot}$	4.41 $\pm$ 0.09	1.96 $\pm$ 0.22
$M_{\rm bol}$	-6.28 $\pm$ 0.22	-0.14 $\pm$ 0.55
B.C.	-2.45	-0.79
M_V	-3.83 $\pm$ 0.25	0.65 $\pm$ 0.52
(m-M)	12.23 $\pm$ 0.22
Distance (pc)	2800 $\pm$ 300

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and reduction
	3 Ephemeris and period analysis
	4 Spectroscopic analysis
	5 Photometric analysis
	6 Absolute dimensions and evolutionary status
	7 Conclusions
	References