The binary nature of the Galactic centre X-ray source CXOGC J174536.1-285638

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Table 3:

Summary of the properties of CXO J17545-28 in comparison to magnetic O and WR and Of?p stars.
ID	Spec.	log( $L_{\rm bol}$ )	log( $L_{\rm x}$ )	log( $L_{\rm x}$ / $L_{\rm bol}$ )	Ref.
	type	(erg s^-1)	(erg s^-1)
CXO J1745-28	WN9h	39.8	35.0	-4.8	1, this study

$\theta^1$ Ori C	O7 V	39.0	33.0	-6.0	2,3,4
$\zeta$ Ori A	O9.7Ib	38.8	32.1	-6.7	5,6
HD 108	O4f?p $\leftrightarrow$ O8.5fp	39.2	33.1	-6.1	2,3
HD 148937	O5.5-6f?p	39.3	33.3	-6.0	3,7
HD 152408 (=WR 79a)	WN9ha	39.6	31.9	-7.7	8
HD 164794	O4 V((f))	39.5	33.1	-6.4	9
HD 191612	O6.5f?pe $\leftrightarrow$ O8fp	39.1	32.9	-6.1	2

Note that no magnetic field determinations have been made for HD 108, while HD 164974 (=9 Sgr) is a suspected CWB. References for this table are: (1) Mikles et al. (2006); (2) Náze et al. (2007); (3) Náze et al. (2008b); (4) Gagné et al. (2005); (5) Raassen et al. (2008); (6) Bouret et al. (2008); (7) Náze et al. (2008c); (8) Oskinova (2005); and (9) Rauw et al. (2002).

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