Variability of massive stars with known spectral types in the Small Magellanic Cloud using 8 years of OGLE-III data

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Table 2

Known eclipsing binaries in the SMC.

#	Star name	Spectral type	RA (J2000)	Dec (J2000)	Skewness	Kurtosis	OGLE-III ID	⟨ I ⟩	⟨ V ⟩	Reference	Period (days)	Note


43	flames1101;SMC5_028846	B0.5:	14.812408	−72.19310	2.998	10.102	SMC108.2.37672	15.92	15.78	W04	3.104372	AM
44	flames1097;SMC5_006928	B0.5:+early B	14.601738	−72.09236	1.891	2.722	SMC108.3.109	16.05	15.81	S07	1.471118	SB2^*
45	AzV204;2dFS1305	B0.5III	14.591625	−72.58792	0.649	−0.437	SMC105.4.16	14.50	14.47	W04	5.844730
46	2dFS2283	B0.5IV	16.839792	−72.20733	1.338	1.370	SMC113.2.24785	14.87	14.60	F07	2.044898
47	2dFS0757	B0.5V	12.577125	−72.64892	0.976	−0.312	SMC101.2.20	15.26	15.10	F07	1.839888
48	NGC330-030;SMC5_020391	B0.5V	14.098250	−72.35657	1.644	1.566	SMC108.8.50687	15.15	14.99	F07	2.320057	SB^**
49	NGC330-055;SMC5_012510	B0.5V	14.205167	−72.49138	0.519	1.002	SMC105.5.37411	15.85	15.67	W04	4.646085
50	2dFS2090	B0.5V	16.490167	−72.19814	0.615	0.546	SMC113.2.16414	15.27	15.01	F07	1.420025	+TEB^a
51	AzV44	B0IIWW	12.197625	−73.41650	0.913	−0.412	SMC100.8.14628	13.90	13.68	W04	1.840730
52	2dFS0498	B0IV	11.036000	−73.23811	2.881	7.994	SMC125.3.41165	14.52	14.39	W04	6.051906	AM

Notes. Full Table 2 is available at the CDS. A portion is shown here for guidance regarding its form and content. (AM) Apsidal Motion, (TEB) Transient EB,

^(*)

Hunter et al. (in prep.),

^(**)

Evans et al. (2006).

^(a)

Additional transient EB with P = 5.242314 days, in the HJD range 2 453 200−2 453 800.

Reference. (W04) Wyrzykowski et al. (2004); (F07) Faccioli et al. (2007); (N02) Niemela et al. (2002); (U98) Udalski et al. (1998); (G05) Groenewegen (2005); (H03) Harries et al. (2003); (H05) Hilditch et al. (2005); (B02) Bayne et al. (2002); (S09) Samus et al. (2009); (M06) Mennickent et al. (2006).

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