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Table 2

Comparison of SAX J2239.3 + 6116 with other Be/X-ray binaries.

X-ray Optical Spectral Disk-loss Porb Inclination vsini Reference
source counterpart type episodes (days) angle (°) (km s-1)

SAX J2239.3 + 6116 B0V no 262.6 25–35 195±20 This work
4U 0115+634 V635 Cas B0.2V yes 24.3 43 300±50 1
RX J0146.9+6121 LS I +61 235 B1V no 200±30 2
V 0332+53 BQ Cam O8-9V no 34.2 <10 <150 3
X Per HD 24534 O9.5III yes 250 23–30 215±10 4, 5
RX J0440.9+4431 LS V +44 17 B1III-V yes 150 235±15 6, 7
1A 0535+262 HD 245770 O9.7III yes 111 28–35 225±10 8, 9
IGR J06074+2205 B0.5IV yes 260±20 10
RX J0812.4-3114 LS 992 B0.5III-V yes 81.3 240±20 11
1A 1118-615 Hen 3-640 O9.5IV no 24 15 ~300 12, 13
4U 1145-619 V801 Cen B0.2III no 187 <45 250±30 14, 15
4U 1258-61 V850 Cen B2V yes 132 shell <600 16
SAX J2103.5+4545 B0V yes 12.7 240±20 17
IGR J21343+4738 B1IV yes shell 365±15 18

Notes. : Shell stars are believed to be equator-on systems, i.e. i ~ 90°.

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